ABO genes are differentially distributed in socio-economic groups in England

No direct evidence is available concerning what average genetic differences, if any, characterize the segments of socially stratified human populations, although theoretical considerations suggest that genetic differentiation within such populations is to be expected. We have now analysed two large samples of data from blood donors in England to test whether the distributions of the ABO and Rhesus blood group phenotypes are random with respect to socio-economic groups as determined by occupational classification. We have found that in both native and migrant sections of the populations of two widely separated regions (south-west England and part of Yorkshire) and in both sexes, the A phenotype is highly significantly more, and the O phenotype significantly less, frequent than expected in social classes I and II, while the converse is seen in social classes III-V. An individual of the A phenotype has thus about 15% greater probability than chance would dictate of being placed in classes I and II. The distribution of the Rh+ and Rh- phenotypes does not differ significantly between classes. It seems unlikely that this nonrandom distribution of the ABO phenotypes among socio-economic groups results from sampling, historical or migrational effects and we conclude that the observed association is likely to result from pleiotropic effects of the ABO alleles (or genes closely linked to them) on attributes influencing occupational type, social mobility and social class.     

A genetic study of intergradation betweenMytilus edulis andMytilus galloprovincialis

Summary A study of geographic variation at 2 diagnostic allozyme loci in the musselsMytilus edulis andM. galloprovincialis reveals considerable spatial variation, both in allele frequencies and in the extent of intergradation.This work was supported in part by grant GR3/2452 from the NERC. We thank M. Hunt, A. Dunn and M. Newton for technical assistance and the many people who gave advice or helped in the collection of specimens.     

A short gamma-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225

Gamma-ray bursts (GRBs) come in two classes: long (> 2 s), soft-spectrum bursts and short, hard events. Most progress has been made on understanding the long GRBs, which are typically observed at high redshift (z approximately 1) and found in subluminous star-forming host galaxies. They are likely to be produced in core-collapse explosions of massive stars. In contrast, no short GRB had been accurately (< 10') and rapidly (minutes) located. Here we report the detection of the X-ray afterglow from--and the localization of--the short burst GRB 050509B. Its position on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225, which is the location one would expect if the origin of this GRB is through the merger of neutron-star or black-hole binaries. The X-ray afterglow was weak and faded below the detection limit within a few hours; no optical afterglow was detected to stringent limits, explaining the past difficulty in localizing short GRBs.     

Relativistic jet activity from the tidal disruption of a star by a massive black hole

Supermassive black holes have powerful gravitational fields with strong gradients that can destroy stars that get too close, producing a bright flare in ultraviolet and X-ray spectral regions from stellar debris that forms an accretion disk around the black hole. The aftermath of this process may have been seen several times over the past two decades in the form of sparsely sampled, slowly fading emission from distant galaxies, but the onset of the stellar disruption event has not hitherto been observed. Here we report observations of a bright X-ray flare from the extragalactic transient Swift J164449.3+573451. This source increased in brightness in the X-ray band by a factor of at least 10,000 since 1990 and by a factor of at least 100 since early 2010. We conclude that we have captured the onset of relativistic jet activity from a supermassive black hole. A companion paper comes to similar conclusions on the basis of radio observations. This event is probably due to the tidal disruption of a star falling into a supermassive black hole, but the detailed behaviour differs from current theoretical models of such events.     

Prolactin concentrations in mouse milk during lactation

Summary Prolactin levels in mouse milk increased from the day of parturition to give a concentration of 230 ng/ml on days 2 and 3 of lactation. Thereafter, levels dropped to 140 ng/ml by day 6 and were maintained at this concentration until weaning.Acknowledgments. Mouse PRL and its antiserum was the generous gift of Y.N. Sinha (Scripps Clinic and Research Foundation, La Jolla, California). J.M.B. was in receipt of a Liverpool University Studentship.     

Understanding the limits to generalizability of experimental evolutionary models

Given the difficulty of testing evolutionary and ecological theory in situ, in vitro model systems are attractive alternatives; however, can we appraise whether an experimental result is particular to the in vitro model, and, if so, characterize the systems likely to behave differently and understand why? Here we examine these issues using the relationship between phenotypic diversity and resource input in the T7-Escherichia coli co-evolving system as a case history. We establish a mathematical model of this interaction, framed as one instance of a super-class of host-parasite co-evolutionary models, and show that it captures experimental results. By tuning this model, we then ask how diversity as a function of resource input could behave for alternative co-evolving partners (for example, E. coli with lambda bacteriophages). In contrast to populations lacking bacteriophages, variation in diversity with differences in resources is always found for co-evolving populations, supporting the geographic mosaic theory of co-evolution. The form of this variation is not, however, universal. Details of infectivity are pivotal: in T7-E. coli with a modified gene-for-gene interaction, diversity is low at high resource input, whereas, for matching-allele interactions, maximal diversity is found at high resource input. A combination of in vitro systems and appropriately configured mathematical models is an effective means to isolate results particular to the in vitro system, to characterize systems likely to behave differently and to understand the biology underpinning those alternatives.     

An age factor affecting variance of a behavioural character in F1 hybrids between inbred lines of the house mouse

Zusammenfassung Eines der Nestbauverhaltenselemente bei Mäusen (Beknappern von Papierstreifen) wurde bei 2 Inzuchtstämmen und deren F₁- und F₂ Hybriden verglichen. F₁-Tiere zeigten im Vergleich zu den Eltern eine grössere Variationsbreite des Verhaltenselementes. Ein grosser und besonders signifikanter Teil dieser Variabilität war einer altersabhängigen Verschiebung zuzuschreiben. Diese kommt wahrscheinlich nicht infolge eines Lernprozesses zustande, sondern durch Änderungen der genetisch-regulierenden Mechanismen (wie. z.B. Dominanz und Epistasie).

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Research supported by a grant from the Netherlands Organization for the Advancement of Pure Research (Z.W.O.). The authors are grateful to MissG. J. Blokzijl for help in making the German summary.     

A genetic study of intergradation between Mytilus edulis and Mytilus galloprovincialis

A study of geographic variation at 2 diagnostic allozyme loci in the mussels Mytilus edultis and M. galloprovincialis reveals considerable spatial variation, both in allele frequencies and in the extent of intergradation.