Atmospheric emission from hydrogen-shell-burning white dwarfs as supersoft X-ray sources

Monthly Notices of the Royal Astronomical Society

Volumn 315, Issue 2, 2000, Pages 345-355

  Shimura, Toshiya ^a  

^a YOKOHAMA NATIONAL UNIVERSITY   (Japan)

Author keywords

Radiative transfer; White dwarfs; X rays: stars

Indexed keywords

ATOMS; COHERENT SCATTERING; COMPTON SCATTERING; ELECTRON SOURCES; HYDROGEN; INCOHERENT SCATTERING; WHITE DWARFS; X RAY APPARATUS;

ABSORPTION EDGES; ABSORPTION FEATURES; ATMOSPHERIC EMISSION; EMISSION ABSORPTION; HYDROSTATIC EQUILIBRIUM; RADIATION SPECTRUM; RADIATIVE EQUILIBRIUM; SPECTRA'S; X-RAY SOURCES; X-RAY:STARS;

RADIATIVE TRANSFER;

EID: 0007503994     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03428.x     Document Type: Article

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