Moderately Thermophilic Magnetotactic Bacteria from Hot Springs in Nevada

Populations of a moderately thermophilic magnetotactic bacterium were discovered in Great Boiling Springs, Nevada, ranging from 32 to 63°C. Cells were small, Gram-negative, vibrioid to helicoid in morphology, and biomineralized a chain of bullet-shaped magnetite magnetosomes. Phylogenetically, based on 16S rRNA gene sequencing, the organism belongs to the phylum Nitrospirae.Magnetotactic bacteria are a metabolically, morphologically, and phylogenetically heterogeneous group of prokaryotes that passively align and actively swim along magnetic field lines (3). This behavior, called magnetotaxis, is due to the presence of intracellular, membrane-bounded, single-magnetic-domain crystals of magnetite (Fe₃O₄) and/or greigite (Fe₃S₄) (3).Most known cultured magnetotactic bacteria are mesophilic and do not grow much above 30°C (e.g., Magnetospirillum species and Desulfovibrio magneticus strains MV-1 and MC-1 [D. A. Bazylinski, unpublished data]). Uncultured magnetotactic bacteria have been observed in numerous habitats that were mostly at 30°C and below. There is only one report describing thermophilic magnetotactic bacteria despite a number of efforts to look for them (e.g., in hydrothermal vents [D. A. Bazylinski, unpublished data]). Nash (12) reported the presence of thermophilic magnetotactic bacteria in microbial mats at about 45 to 55°C adjacent to the main flow in Little Hot Creek (but not in other springs in the same area at 40 to 80°C) and in microbial mats of other springs in central California at up to 58°C, all on the east side of the Sierra Nevada mountains. Cells biomineralized bullet-shaped crystals of magnetite and were phylogenetically affiliated with the phylum Nitrospirae (12). Few additional details were provided regarding the organisms and their habitat.In this study, water and surface sediment samples were taken from the Great Boiling Springs (GBS) geothermal field in Gerlach, NV. GBS is a series of hot springs that range from ambient temperature to ∼96°C (2, 5). The geology, chemistry, and microbial ecology of the springs have been described in some detail (2, 5). The pHs of the samples ranged from 6.4 to 7.5, while the salinities were about 4 to 5 ppt, as determined with a handheld Palm Abbe PA203 digital refractometer (MISCO Refractometer, Cleveland, OH). Samples were examined for the presence of magnetotactic bacteria using the hanging drop technique on-site and in the laboratory at room temperature with and without magnetic enrichment of the sample (15). Some samples taken back to the laboratory were kept at an elevated temperature (∼62°C), while others were kept at ambient temperature. There did not appear to be a significant difference in the number of magnetotactic cells in samples taken back to the laboratory and kept at these two temperatures. Only one morphotype of magnetotactic bacteria was found in samples from nine springs whose temperatures ranged from 32 to 63°C, and we estimate their numbers to be between 10³ to 10⁵ cells ml⁻¹ in surface sediments in sample bottles. We did not observe magnetotactic cells of this type in a large number of springs or pools that were at <32°C. Only one spring positive for the presence of these magnetotactic bacteria had sediment that was partially covered with a microbial mat, while sediment at most of the springs was dark gray in color. Cells were small (1.8 ± 0.4 by 0.4 ± 0.1 μm; n = 59), Gram negative, vibrioid to helicoid in morphology, and possessed a single polar flagellum (Fig. ​(Fig.1A).1A). Magnetotactic bacteria were not observed in springs that were at 67°C and above, suggesting the maximum survival and perhaps growth temperature for the organism is about 63°C. In the lab, cells remained viable and motile in samples kept at 25 to 62°C for several months. We refer to this organism as strain HSMV-1.Open in a separate windowFIG. 1.Transmission electron microscope (TEM) images of cells and magnetosomes of strain HSMV-1. (A) TEM image of unstained cell of HSMV-1 showing a single polar flagellum and a single chain of bullet-shaped magnetosomes. The electron-dense structures at the poles were found to be phosphorus-rich based on energy-dispersive X-ray analysis (data not shown) and therefore likely represent polyphosphate granules. (B) Higher-magnification TEM image of the magnetosome chain. (C) High-magnification TEM image of magnetosomes from which a selected area electron diffraction (SAED) pattern was obtained (inset of B). The SAED pattern corresponds to the [1 0−1] zone of magnetite, Fe₃O₄: reflection o, (0 0 0); reflection a, (1 −1 1) (0.48 nm); reflection b, (1 1 1) (0.48 nm); reflection c, (2 0 2) (0.30 nm); angle a-o-b, 70.5°. (D) Iron, sulfur, and oxygen elemental maps, derived from energy-filtering transmission electron microscopy (EFTEM), showing that the positions of the magnetosome crystals correlate with increased concentrations of Fe and O, but not S, consistent with the iron oxide magnetite (Fe₃O₄).Cells of HSMV-1 biomineralized a single chain of magnetosomes that traversed the cells along their long axis (Fig. 1A to C). Selected area electron diffraction (SAED) and energy-filtering transmission electron microscopy (EFTEM) elemental maps were determined on magnetosome crystals using a Tecnai model G2 F30 Super-Twin transmission electron microscope (FEI Company, Hillsboro OR). SAED patterns of HSMV-1 magnetosome crystals (Fig. ​(Fig.1B,1B, inset) indicated that they consisted of magnetite, while EFTEM elemental maps (Fe, O and S) (Fig. ​(Fig.1D)1D) clearly showed that the crystals consisted of an iron oxide and not an iron sulfide, again consistent with the mineral magnetite. Cells contained an average of 12 ± 6 magnetosome crystals per cell (n = 15 cells) that averaged 113 ± 34 by 40 ± 5 nm in size (n = 179). A plot of the length of the crystals as a function of the shape factor (width/length ratio) is provided in Figure S1 in the supplemental material and shows that the crystals fit in the theoretical single-magnetic-domain size range (4), along with all known mature magnetosome magnetite crystals from magnetotactic bacteria (3).Whole-cell PCR amplification of the 16S rRNA gene was performed by first magnetically purifying cells of HSMV-1 using the “capillary racetrack” described by Wolfe et al. (18). Purity of the collected cells was determined by microscopic examination, and contaminating cells were never observed. The 16S rRNA gene was amplified using bacteria-specific primers 27F 5′-AGAGTTTGATCMTGGCTCAG-3′ and 1492R 5′-TACGGHTACCTTGTTACGACTT-3′ (11). PCR products were cloned into pGEM-T Easy vector (Promega Corporation, Madison, WI) and sequenced (Functional Biosciences, Inc., Madison, WI). Six of eight clones sequenced had identical inserts.Alignment of 16S rRNA gene sequences was performed using the CLUSTAL W multiple alignment accessory application in the BioEdit sequence alignment editor (7). Phylogenetic trees were constructed using MEGA version 4 (17) by applying the neighbor-joining method (14). Bootstrap values were calculated with 1,000 replicates. The 16S rRNA gene sequence of strain HSMV-1 places the organism in the phylum Nitrospirae (Fig. ​(Fig.2),2), with its closest relative in culture being Thermodesulfovibrio hydrogeniphilus (87.2% identity) (8). Two other uncultured magnetotactic bacteria are phylogenetically affiliated with the phylum Nitrospirae, including the unnamed rod-shaped bacterium strain MHB-1 (86.5% identity) (6) and the very large Candidatus Magnetobacterium bavaricum (86.4% identity) (16). Interestingly, all the magnetotactic bacteria associated with the phylum Nitrospirae thus far (e.g., Candidatus Magnetobacterium bavaricum) contain bullet-shaped magnetite crystals in their magnetosomes.Open in a separate windowFIG. 2.Phylogenetic tree based on 16S rRNA gene sequences showing the phylogenetic position of strain HSMV-1 in the phylum Nitrospirae. Bootstrap values at nodes are percentages of 1,000 replicates. The magnetotactic bacteria Desulfovibrio magneticus and Candidatus Magnetoglobus multicellularis (outgroup; deltaproteobacteria) were used to root the tree. GenBank accession numbers are given in parentheses. Bar represents 2% sequence divergence.Fluorescent in situ hybridization (FISH) was used to authenticate the 16S rRNA gene sequence. A specific Alexa594-labeled probe for HSMV-1 was designed (HSMVp, 5′-CCTTCGCCACAGGCCTTCTA-3′, complementary to nucleotides 690 to 709 of the 16S rRNA molecule) based on the alignment of 10 of the most similar 16S rRNA gene sequences found in GenBank after BLAST analysis (1) and on cultivated members of the phylum Nitrospirae. FISH with the Alexa594-labeled probe was carried out after fixation of magnetically concentrated cells directly on the wells of gelatin-coated hydrophobic microscope slides with 4% paraformaldehyde. FISH was performed according to the work of Pernthaler et al. (13). The hybridization solution contained 10 ng/ml of the probe, 20% formamide, 0.9 M NaCl, 20 mM Tris-HCl (pH 7.4), 1 mM Na₂EDTA, and 0.01% sodium dodecyl sulfate (SDS). Cells of HSMV-1 hybridized to the HSMVp probe, while other cells in the sample did not (Fig. ​(Fig.3),3), indicating that the 16S rRNA gene sequence we obtained is from the magnetotactic bacterium under study. Strain HSMV-1 clearly represents a new genus (Fig. ​(Fig.2),2), and based on the phylogeny and what we currently know phenotypically about strain HSMV-1, we propose the name Candidatus Thermomagnetovibrio paiutensis (the GBS site was originally occupied by the Paiute Indian Tribe).Open in a separate windowFIG. 3.Fluorescent in situ hybridization (FISH) of cells of strain HSMV-1 using an HSMV-1-specific oligonucleotide rRNA probe (HSMVp). Cells used for FISH were magnetically concentrated by placing a magnet next to the side of the sample bottle for 30 min and then removed with a Pasteur pipette. This technique was used rather than the magnetic racetrack method in order to have many HSMV-1 cells as well as some other cells that could be used as a negative control. (A) Differential interference contrast (DIC) image of HSMV-1 cells (filled arrows) and other cells (negative control; empty arrows) from hot spring samples; (B) cells stained with 4′,6-diamidino-2-phenylindole (DAPI); (C) cells hybridized with the specific probe HSMVp.Nash (12) first reported thermophilic magnetotactic bacteria phylogenetically affiliated with the Nitrospirae phylum in hot springs, and it would be interesting and important to compare these organisms and their habitats. However, little can be compared at this time due to lack of information. Nash (12) reported that the one spring at Little Hot Creek was freshwater and that microbial mats were present at all springs where thermophilic magnetotactic bacteria were found. The water at our sampling sites was brackish, not freshwater, and microbial mats were not an important feature of our springs. Thus, it is difficult to determine without knowing the relationship between the organisms found by Nash (12) and strain HSMV-1 what environmental parameters are important to the growth and survival of these bacteria.It is also difficult to determine the temperature ranges for the survival and growth for strain HSMV-1 without having a pure culture. Data presented here suggest that the temperature range for both is quite wide, and this would be important for the continued presence of HSMV-1 at GBS, as temperatures in the hot springs are known to fluctuate greatly (2). Even if the maximum growth temperature of HSMV-1 is slightly lower than the maximum survival temperature (a conservative estimate) that we know of (63°C), it would still be considered a moderately thermophilic bacterium.The results presented here clearly show that some magnetotactic bacteria can be considered at least moderately thermophilic. They extend the upper temperature limit for environments where magnetotactic bacteria exist and likely grow (∼63°C) and where magnetosome magnetite is deposited, a finding that may prove significant in the study and interpretation of magnetofossils (9, 10).     

Cranioectodermal Dysplasia, Sensenbrenner Syndrome, Is a Ciliopathy Caused by Mutations in the IFT122 Gene

Cranioectodermal dysplasia (CED) is a disorder characterized by craniofacial, skeletal, and ectodermal abnormalities. Most cases reported to date are sporadic, but a few familial cases support an autosomal-recessive inheritance pattern. Aiming at the elucidation of the genetic basis of CED, we collected 13 patients with CED symptoms from 12 independent families. In one family with consanguineous parents two siblings were affected, permitting linkage analysis and homozygosity mapping. This revealed a single region of homozygosity with a significant LOD score (3.57) on chromosome 3q21-3q24. By sequencing candidate genes from this interval we found a homozygous missense mutation in the IFT122 (WDR10) gene that cosegregated with the disease. Examination of IFT122 in our patient cohort revealed one additional homozygous missense change in the patient from a second consanguineous family. In addition, we found compound heterozygosity for a donor splice-site change and a missense change in one sporadic patient. All mutations were absent in 340 control chromosomes. Because IFT122 plays an important role in the assembly and maintenance of eukaryotic cilia, we investigated patient fibroblasts and found significantly reduced frequency and length of primary cilia as compared to controls. Furthermore, we transiently knocked down ift122 in zebrafish embryos and observed the typical phenotype found in other models of ciliopathies. Because not all of our patients harbored mutations in IFT122, CED seems to be genetically heterogeneous. Still, by identifying CED as a ciliary disorder, our study suggests that the causative mutations in the unresolved cases most likely affect primary cilia function too.     

Echinocystic acid 3,16-O-bisglycosides from Albizia procera

Three triterpene glycosides and two known ones were isolated from the bark of Albizia procera by using chromatographic techniques. The structures of the compounds were determined to be 3-O-β-d-xylopyranosyl-(1 → 2)-β-d-galactopyranosyl-(1 → 6)-2-acetamido-2-deoxy-β-d-glucopyranosyl echinocystic acid 16-O-β-d-glucopyranoside, 3-O-β-d-xylopyranosyl-(1 → 2)-α-l-arabinopyranosyl-(1 → 6)-2-acetamido-2-deoxy-β-d-glucopyranosyl echinocystic acid 16-O-β-d-glucopyranoside and 3-O-α-l-arabinopyranosyl-(1 → 2)-α-l-arabinopyranosyl-(1 → 6)-2-acetamido-2-deoxy-β-d-glucopyranosyl echinocystic acid 16-O-β-d-glucopyranoside. Their structures were determined by NMR techniques including HOHAHA, ¹H-¹H COSY, ROE, HMQC and HMBC experiments together with FABMS as well as acid hydrolysis. To the best of our knowledge, the new compounds are considered the first examples of echinocystic acid 3,16-O-bisglycosides. In contrast to other cytotoxic echinocystic acid glycosides with N-acetyl glucosamine unit, the new glycosides were found inactive when assayed by MTT method for their cytotoxicities against the human tumor cell lines HEPG2, A549, HT29 and MCF7. The results showed the importance of the free hydroxyl group at the aglycone C-16 for exhibiting cytotoxic properties.     

Sampling Protein Form and Function with the Atomic Force Microscope

To study the structure, function, and interactions of proteins, a plethora of techniques is available. Many techniques sample such parameters in non-physiological environments (e.g. in air, ice, or vacuum). Atomic force microscopy (AFM), however, is a powerful biophysical technique that can probe these parameters under physiological buffer conditions. With the atomic force microscope operating under such conditions, it is possible to obtain images of biological structures without requiring labeling and to follow dynamic processes in real time. Furthermore, by operating in force spectroscopy mode, it can probe intramolecular interactions and binding strengths. In structural biology, it has proven its ability to image proteins and protein conformational changes at submolecular resolution, and in proteomics, it is developing as a tool to map surface proteomes and to study protein function by force spectroscopy methods. The power of AFM to combine studies of protein form and protein function enables bridging various research fields to come to a comprehensive, molecular level picture of biological processes. We review the use of AFM imaging and force spectroscopy techniques and discuss the major advances of these experiments in further understanding form and function of proteins at the nanoscale in physiologically relevant environments.To understand biological processes at the molecular level it is essential to identify the involved proteins and proteinaceous assemblies, to characterize their structure and function, and to unravel their interplay with other proteins and molecules (1). Techniques like x-ray crystallography, electron microscopy, nuclear magnetic resonance spectroscopy, and mass spectrometry have contributed massively to elucidate such protein properties. These techniques can easily sample the properties of a large ensemble of proteins; however, they require subjecting the sample to harsh treatments such as drying, crystallizing, or vaporizing in vacuum, thereby limiting the range of measurable dynamical properties of the sample. One powerful method that permits the investigation of molecules in their native physiological buffer condition is atomic force microscopy (AFM)¹ (2). An atomic force microscope is a microscope and force spectrometer at the same time. The imaging resolution of the atomic force microscope is comparable with that of electron microscopes, and it has the special capability to image samples in a variety of environments such as in vacuum, air, or liquid, which therefore enables studying biological specimens in their native environments (i.e. in buffer solutions) (3, 4). In addition, its ability to “touch” the sample gives it the advantage to manipulate single particles/molecules and probe their mechanical properties (5–8). However, AFM force spectroscopy is currently a technique with rather fast pulling and pushing speeds, thereby often operating out of equilibrium conditions. Improvements with ultrastable atomic force microscopes are underway to tackle this problem with promising results (9, 10). Furthermore, AFM is not well suited to apply and resolve forces at the single piconewton range due to large size tips and relatively stiff cantilevers. The issue of nonspecificity of the tip interaction with the sample is also of concern, especially in pulling experiments that require the capability to accurately recognize and select the appropriate molecule or point of interest. The current introduction of carbon nanotube tips can address the former issue (11, 12), whereas techniques in chemical functionalization can provide directed tip specificity and recognition capability (13–18), thereby further improving and widening the applicability of AFM in the future. In addition, the coupling of the atomic force microscope to fluorescence microscopes further enhances its versatility by adding (single molecule) fluorescence imaging to the AFM imaging capability (19–21), and the development of high speed systems makes it possible for AFM to probe fast dynamics of various biological processes (22–26).The applicability of AFM in proteomics is diverse and includes the characterization of the cell surface proteome (for a recent review, see Ref. 27), label-free detection and counting of single proteins (28, 29), and force spectroscopy measurements of binding and unbinding events (30, 31). In structural biology, AFM has shown to be a powerful tool for high resolution imaging of proteins in near native conditions (3, 6) and structural studies of supramolecular assemblies like protein filaments and viruses by nanoindentation methods (32, 33). These experiments show the potential of AFM to study both “form” and “function” of proteins, thereby resolving questions in proteomics and structural biology quasi-simultaneously. In the following, we will explain the principles of atomic force microscopy and its different operation modes and finally discuss examples of imaging, nanoindentation, and protein (un)binding and unfolding studies using AFM.     

Major Radiodiagnostic Imaging in Pregnancy and the Risk of Childhood Malignancy: A Population-Based Cohort Study in Ontario

Background

The association between fetal exposure to major radiodiagnostic testing in pregnancy—computed tomography (CT) and radionuclide imaging—and the risk of childhood cancer is not established.

Methods and Findings

We completed a population-based study of 1.8 million maternal-child pairs in the province of Ontario, from 1991 to 2008. We used Ontario''s universal health care–linked administrative databases to identify all term obstetrical deliveries and newborn records, inpatient and outpatient major radiodiagnostic services, as well as all children with a malignancy after birth. There were 5,590 mothers exposed to major radiodiagnostic testing in pregnancy (3.0 per 1,000) and 1,829,927 mothers not exposed. The rate of radiodiagnostic testing increased from 1.1 to 6.3 per 1,000 pregnancies over the study period; about 73% of tests were CT scans. After a median duration of follow-up of 8.9 years, four childhood cancers arose in the exposed group (1.13 per 10,000 person-years) and 2,539 cancers in the unexposed group (1.56 per 10,000 person-years), a crude hazard ratio of 0.69 (95% confidence interval 0.26–1.82). After adjusting for maternal age, income quintile, urban status, and maternal cancer, as well as infant sex, chromosomal or congenital anomalies, and major radiodiagnostic test exposure after birth, the risk was essentially unchanged (hazard ratio 0.68, 95% confidence interval 0.25–1.80).

Conclusions

Although major radiodiagnostic testing is now performed in about 1 in 160 pregnancies in Ontario, the absolute annual risk of childhood malignancy following exposure in utero remains about 1 in 10,000. Since the upper confidence limit of the relative risk of malignancy may be as high as 1.8 times that of an unexposed pregnancy, we cannot exclude the possibility that fetal exposure to CT or radionuclide imaging is carcinogenic. Please see later in the article for the Editors'' Summary     

Dependence of the Q10 values on the depth of the soil temperature measuring point

The parameter Q₁₀ is commonly used to express the relationship between soil CO₂ efflux and soil temperature. One advantage of this parameter is its application in a model expression of respiration losses of different ecosystems. Correct specification of Q₁₀ in these models is indispensable. Soil surface CO₂ efflux and soil temperature at different depths were measured in a 21-year-old Norway spruce stand and a mountain grassland site located at the Experimental Ecological Study Site Bily Kriz, Beskydy Mts. (NE Czech Republic), using automated gasometric systems. A time-delay and goodness-of-fit between soil CO₂ efflux and soil temperature at different measuring depths were determined. Wide ranges of values for the time-delay of CO₂ efflux in response to temperature, Q₁₀ and the determination coefficient (R²) between CO₂ efflux and temperature were obtained at the both sites. The values of Q₁₀ and the CO₂ time-delay increased with depth, while the R² of the CO₂-temperature relationship significantly decreased. Soil temperature records obtained close to the soil surface showed the highest values of R² and the lowest value of the time-delay at both sites. Measurement of soil temperature at very shallow soil layer, preferably at the soil surface, is highly recommended to determine useable values of Q₁₀. We present a new procedure to normalize Q₁₀ values for soil temperatures measured at different depths that would facilitate comparison of different sites.     

Different defense strategies of Dendrolimus pini, Galleria mellonella, and Calliphora vicina against fungal infection

The resistance of Galleria mellonella, Dendrolimus pini, and Calliphora vicina larvae against infection by the enthomopathogen Conidiobolus coronatus was shown to vary among the studied species. Exposure of both G. mellonella and D. pini larvae to the fungus resulted in rapid insect death, while all the C. vicina larvae remained unharmed. Microscopic studies revealed diverse responses of the three species to the fungal pathogen: (1) the body cavities of D. pini larvae were completely overgrown by fungal hyphae, with no signs of hemocyte response, (2) infected G. mellonella larvae formed melanotic capsules surrounding the fungal pathogen, and (3) the conidia of C. coronatus did not germinate on the cuticle of C. vicina larvae. The in vitro study on the degradation of the insect cuticle by proteases secreted by C. coronatus revealed that the G. mellonella cuticle degraded at the highest rate. The antiproteolytic capacities of insect hemolymph against fungal proteases correlated well with the insects' susceptibility to fungal infection. The antiproteolytic capacities of insect hemolymph against fungal proteases correlated well with the insects' susceptibility to fungal infection. Of all the tested species, only plasmatocytes exhibited phagocytic potential. Exposure to the fungal pathogen resulted in elevated phagocytic activity, found to be the highest in the infected G. mellonella. The incubation of insect hemolymph with fungal conidia and hyphae revealed diverse reactions of hemocytes of the studied insect species. The encapsulation potential of D. pini hemocytes was low. Hemocytes of G. mellonella showed a high ability to attach and encapsulate fungal structures. Incubation of C. vicina hemolymph with C. coronatus did not result in any hemocytic response. Phenoloxidase (PO) activity was found to be highest in D. pini hemolymph, moderate in G. mellonella, and lowest in the hemolymph of C. vicina. Fungal infection resulted in a significant decrease of PO activity in G. mellonela larvae, while that in the larvae of D. pini remained unchanged. PO activity in C. vicina exposed to fungus slightly increased. The lysozyme-like activity increased in the plasma of all three insect species after contact with the fungal pathogen. Anti E. coli activity was detected neither in control nor in infected D. pini larvae. No detectable anti E. coli activity was found in the control larvae of G. mellonella; however, its exposure to C. coronatus resulted in an increase in the activity to detectable level. In the case of C. vicina exposure to the fungus, the anti E. coli activity was significantly higher than in control larvae. The defense mechanisms of D. pini (species of economic importance in Europe) are presented for the first time.     

Effects of implant design parameters on fluid convection, potentiating third-body debris ingress into the bearing surface during THA impingement/subluxation

Aseptic loosening from polyethylene wear debris is the leading cause of failure for metal-on-polyethylene total hip implants. Third-body debris ingress to the bearing space results in femoral head roughening and acceleration of polyethylene wear. How third-body particles manage to enter the bearing space between the closely conforming articulating surfaces of the joint is not well understood. We hypothesize that one such mechanism is from convective fluid transport during subluxation of the total hip joint. To test this hypothesis, a three-dimensional (3D) computational fluid dynamics (CFD) model was developed and validated, to quantify fluid ingress into the bearing space during a leg-cross subluxation event. The results indicated that extra-articular joint fluid could be drawn nearly to the pole of the cup with even very small separations of the femoral head (<0.60mm). Debris suspended near the equator of the cup at the site of maximum fluid velocity just before the subluxation began could be transported to within 11 degrees from the cup pole. Larger head diameters resulted in increased fluid velocity at all sites around the entrance to the gap compared to smaller head sizes, with fluid velocity being greatest along the anterosuperolateral cup edge, for all head sizes. Fluid pathlines indicated that suspended debris would reach similar angular positions in the bearing space regardless of head size. Increased inset of the femoral head into the acetabular cup resulted both in higher fluid velocity and in transport of third-body debris further into the bearing space.     

WHAT IS IT TO BE A DAUGHTER? IDENTITIES UNDER PRESSURE IN DEMENTIA CARE

This article concentrates on the care for people who suffer from progressive dementia. Dementia has a great impact on a person’s well‐being as well as on his or her social environment. Dealing with dementia raises moral issues and challenges for participants, especially for family members. One of the moral issues in the care for people with dementia is centred on responsibilities; how do people conceive and determine their responsibilities towards one another? To investigate this issue we use the theoretical perspective of Margaret Walker. She states that ideas about identity play a crucial role in patterns of normative expectations with regard to the distribution of responsibilities in daily practices of care. The results of this study show how the identity of a family‐member is put under pressure and changes during her loved one’s illness that leads to difficulties and misunderstandings concerning the issue of responsibility. These results offer an insight into the complexities of actual practices of responsibility and highlight the importance for those caring for people with dementia of attending carefully to how they see themselves and how they see other people involved (Who am I? Who do I want to be for the other?). Answers to such questions show what people expect from themselves and from one another, and how they, at any rate, are distributing responsibilities in a given situation. Professional caregivers should take into account that family members might have different ideas about who they are and consequently about what their responsibilities are.