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  • ASTROPHYSICS  (1)
  • Cell & Developmental Biology  (1)
  • 1
    ISSN: 0148-7280
    Keywords: spermatozoa ; acrosomal membrane ; membrane antigens ; Life and Medical Sciences ; Cell & Developmental Biology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology
    Notes: Antiserum to purified boar spermatozoan outer acrosomal membrane (OAM) was raised in rabbits and adsorbed with boar liver and serum glutaraldehyde cross-linked immunoadsorbents. The IgG fraction of the antiserum was purified by (NH4)2SO4 precipitation followed by ion-exchange chromatography. Indirect immunofluorescence showed bright fluorescent staining of the acrosomal cap of boar spermatozoa and to a lesser extent of the acrosomes of bull and goat spermatozoa after incubation with anti-OAM-IgG. Immuno-electron microscopy further confirmed the specificity of the antibody for the OAM. Preincubation of the anti-OAM-IgG with isolated OAM, completely abolished its reactivity. When tested by ELISA, anti-OAM-IgG reacted with boar, bull, goat, and human spermatozoa; however, its binding activity to boar spermatozoa was significantly greater as compared to spermatozoa from the other species tested.In an effort to identify OAM antigens recognized by this antiserum, the isolated boar OAM was labeled either with 3H or with 125I and solubilized by mild detergent treatment. The extracted components were immunoprecipitated with anti-OAM-IgG and protein A-bearing S. aureus and the thus isolated antigens were analysed on SDS-PAGE. The results suggest that anti-OAM-IgG recognized one high molecular 3H-labeled glycoprotein (270 kd), and four 125I-labeled polypeptides of lower molecular weight of the boar OAM.
    Additional Material: 7 Ill.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2014-09-16
    Description: The discovery of broad P Cygni profiles in early type stars and the detection of X-rays emitted from the envelopes of these stars made it clear, that a considerable amount of mechanical energy has to be present in massive stars. An attack on the problem, which has proven successful when applied to late type stars is proposed. It is possible that acoustic waves form out of random fluctuations, amplify by absorbing momentum from stellar radiation field, steepen into shock waves and dissipate. A stellar atmosphere was constructed, and sinusoidal small amplitude perturbations of specified Mach number and period at the inner boundary was introduced. The partial differential equations of hydrodynamics and the equations of radiation transfer for grey matter were solved numerically. The equation of motion was augmented by a term which describes the absorption of momentum from the radiation field in the continuum and in lines, including the Doppler effect and allows for the treatment of a large number of lines in the radiative acceleration term.
    Keywords: ASTROPHYSICS
    Type: NASA. Goddard Space Flight Center The Origin of Nonradiative Heating(Momentum in Hot Stars; p 233-235
    Format: text
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