Production of the haemopoietic growth factors GM-CSF and interleukin-3 by mast cells in response to IgE receptor-mediated activation

Mast cells have a central role in allergic diseases mediated by specific immunoglobulin E antibody responses to allergens. The binding of IgE to the high-affinity receptor for IgE (Fc epsilon R) on mast cells and basophils enables these cells to react specifically to allergens. Such contact leads to the activation of mast cells and the release of histamine and other pharmacological mediators, causing an immediate hypersensitivity and acute inflammatory reactions, accompanied by the development of allergic symptoms. Here we show that Fc epsilon R-mediated activation of murine mast cells results in the production of the haemopoietic growth factors granulocyte/macrophage colony-stimulating factor (GM-CSF) and interleukin-3 (IL-3). IL-3 and GM-CSF, in addition to their role in bone marrow haemopoiesis, also influence inflammation as they have the capacity to recruit, prime and activate inflammatory cells such as neutrophils, macrophages and eosinophils. Secretion of these factors by mast cells in response to allergens may therefore have an important role in local tissue defense.     

RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system

RR Lyrae pulsating stars have been extensively used as tracers of old stellar populations for the purpose of determining the ages of galaxies, and as tools to measure distances to nearby galaxies. There was accordingly considerable interest when the RR Lyrae star OGLE-BLG-RRLYR-02792 (referred to here as RRLYR-02792) was found to be a member of an eclipsing binary system, because the mass of the pulsator (hitherto constrained only by models) could be unambiguously determined. Here we report that RRLYR-02792 has a mass of 0.26 solar masses M[symbol see text] and therefore cannot be a classical RR Lyrae star. Using models, we find that its properties are best explained by the evolution of a close binary system that started with M[symbol see text] and 0.8M[symbol see text]stars orbiting each other with an initial period of 2.9 days. Mass exchange over 5.4 billion years produced the observed system, which is now in a very short-lived phase where the physical properties of the pulsator happen to place it in the same instability strip of the Hertzsprung-Russell diagram as that occupied by RR Lyrae stars. We estimate that only 0.2 per cent of RR Lyrae stars may be contaminated by systems similar to this one, which implies that distances measured with RR Lyrae stars should not be significantly affected by these binary interlopers.     

Migration rates of human populations from surname distributions

Migration is an important factor in the biological evolution of human populations, and surnames provide one of the simplest records of identification. The distribution of surnames can supply quantitative information on the structure of human populations. Surnames considered as alleles of a gene transmitted only by the male line can be assumed to be neutral markers and therefore satisfy the expectations of the neutral theory of evolution, which is entirely described by random genetic drift, mutation and migration. As data on surnames are easier to collect than those from genes, the information yield is potentially increased, but the validity of the conclusions must be tested in actual samples. The purpose of this report is to compare the estimates of migration rates in Italy, as inferred by the surname distribution found in the telephone directories and other sources, with the corresponding estimates from official demographic sources. Our findings show that in these samples the ratio of surnames to individuals makes it possible to calculate reliable estimates of migration rates.