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  • 1
    ISSN: 1365-2826
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Medicine
    Notes: Lamprey gonadotropin releasing-hormone (LGnRH)-III, a hypothalamic neurohormone recently isolated from sea lamprey, was reported to have a selective stimulatory effect on follicle-stimulating hormone (FSH) release in rats and suggested to be the mammalian FSH-releasing factor. In this study, we determined the relative luteinizing hormone (LH)- and FSH-releasing potency of LGnRH-III compared to mammalian gonadotropin-releasing hormone (LHRH) in normal female rats, ovariectomized (OVX) and oestrogen/progesterone substituted rats and the superfused rat-pituitary cell system. The specificity of LGnRH-III for the mammalian LHRH receptor was investigated by blocking the receptor with an LHRH antagonist, MI-1544. In vitro, LGnRH-III dose-dependently stimulated both LH and FSH secretion from rat pituitary cells at 10−7 to 10−5 M concentrations, while LHRH stimulated gonadotropin secretion at a 1000-fold lower doses (10−10 to 10−8 M). The difference between its LH- and FSH-releasing potency was similar to that of LHRH. LGnRH-III bound to high affinity binding sites on rat pituitary cells with a Kd of 6.7 nm, Bmax=113±27 fmol/mg protein. In vivo, LGnRH-III also stimulated both LH and FSH secretion in a dose-dependent manner and, similar to LHRH, induced a greater rise in the serum LH than the FSH level. In normal cycling rats, it showed 180–650-fold weaker potency than LHRH in stimulating LH secretion and 70–80-fold weaker effect in stimulating FSH secretion. In OVX rats, LGnRH-III demonstrated a similarly weak effect on both gonadotropins. It was found to be 40–210-fold less potent than LHRH regarding LH release and 50–160-fold weaker regarding FSH release. LHRH-receptor antagonist MI-1544 prevented both the LH- and the FSH-releasing effect of LGnRH-III both in vitro and in vivo. These results do not support the hypothesis that LGnRH-III might be the mammalian FSH-releasing factor but demonstrate that it is a weak agonist for the pituitary LHRH receptor and stimulates both gonadotropins in a dose-dependent fashion.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 187 (1992), S. 329-332 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Pion condensates can help to explain a variety of physical properties owned by pulsars if they are present in their interiors. It has been noted that they offer, for example, an attractive alternative to understand glitches by improving former core-quake models. We discuss this scenario and show in this work some constraints on the properties of this type of matter arise from X-ray observations of the Vela pulsar performed by theEinstein Observatory. Further information on this subject will be soon obtained from improved facilities and we expect them to give further constraints to the viability of those models.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 189 (1992), S. 159-162 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We consider a simple qualitative model to estimate the time-scale forneutron→strange matter decay in dense stellar environments. It is argued that a large mismatch between the former and the microscopic weak interaction time-scale suggests that a dual population of both types of compact objects is unlikely. Assuming the correctness of the strange matter hypothesis all of them should be strange stars. If one instead postulates accretion as the decisive feature for the conversion, a consideration of neutron stars structure indicates a fairly narrow range for the onset of the critical density before the corresponding Chandrasekhar mass is achieved.
    Type of Medium: Electronic Resource
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