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  • Astrophysics  (1)
  • Cerebrospinal fluid  (1)
  • 1
    ISSN: 1432-0878
    Keywords: Brain, vertebrate ; Development, ontogenetic ; Proteins, plasma ; Cerebrospinal fluid ; Fetuin ; α2HS glycoprotein ; Human ; Sheep
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Summary The human plasma protein, α2HS glycoprotein, has an amino acid composition very similar to that of fetuin, the major protein in fetal calf and lamb serum. Immunohistochemical studies of human fetuses (6–33 weeks gestation) showed that α2HS glycoprotein and fetuin have similar distributions in developing brain and several other tissues, e.g., bone, kidney, gonads, gastrointestinal tract, respiratory and cardiovascular systems. There were notable differences in the liver and thymus in the distribution of the two proteins. Fetuin and α2HS glycoprotein are present in plasma and cerebrospinal fluid of both human and sheep fetuses; their concentrations are reciprocally related: in human plasma and cerebrospinal fluid α2HS glycoprotein concentration is high and fetuin low; the reverse is the case in sheep fetuses. Estimates of the concentration of α2HS glycoprotein in human fetal cerebrospinal fluid and plasma were obtained. It is suggested that α2HS glycoprotein may play a role in developing tissues, especially in the human fetus, similar to that of fetuin in other species.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-07-13
    Description: We present the results of a NuSTAR study of the dynamically confirmed stellar-mass black hole GS 1354645. The source was observed during its 2015 "hard" state outburst; we concentrate on spectra from two relatively bright phases. In the higher-flux observation, the broadband NuSTAR spectra reveal a clear, strong disk reflection spectrum, blurred by a degree that requires a black hole spin of a = cJ/ GM(sup 2) 〉 or = 0.98 (1(sigma) statistical limits only). The fits also require a high inclination: theta approx. = 75(2)deg. Strong "dips" are sometimes observed in the X-ray light curves of sources viewed at such an angle; these are absent, perhaps indicating that dips correspond to flared disk structures that only manifest at higher accretion rates. In the lower flux observation, there is evidence of radial truncation of the thin accretion disk. We discuss these results in the context of spin in stellar-mass black holes, and inner accretion flow geometries at moderate accretion rates.
    Keywords: Astrophysics
    Type: GSFC-E-DAA-TN41102 , The Astrophysical Journal Letters (ISSN 2041-8205) (e-ISSN 2041-8213); 826; 1; L12
    Format: text
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