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Search: WFRF:(Abramowicz Marek A 1945) > (2015-2019) > Stable, levitating,...

Stable, levitating, optically thin atmospheres of Eddington-luminosity neutron stars

Wielgus, M. (author)
Kluzniak, W. (author)
Sadowski, A. (author)
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Narayan, R. (author)
Abramowicz, Marek A, 1945 (author)
Gothenburg University,Göteborgs universitet,Institutionen för fysik (GU),Department of Physics (GU)
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 (creator_code:org_t)
2015-10-20
2015
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 454:4, s. 3766-3770
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • In general relativity, static gaseous atmospheres may be in hydrostatic balance in the absence of a supporting stellar surface, provided that the luminosity is close to the Eddington value. We construct analytic models of optically thin, spherically symmetric shells supported by the radiation pressure of a luminous central body in the Schwarzschild metric. Opacity is assumed to be dominated by Thomson scattering. The inner parts of the atmospheres, where the luminosity locally has supercritical values, are characterized by a density and pressure inversion. The atmospheres are convectively and Rayleigh-Taylor stable, and there is no outflow of gas. RAMOWICZ MA, 1990, ASTROPHYSICAL JOURNAL, V361, P470

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

gravitation
relativistic processes
stars: atmospheres
stars: neutron
x-ray sources
capture
Astronomy & Astrophysics

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