Hydrogen shell-burning models for RX J0925.7 - 4758

Publications of the Astronomical Society of Japan

Volumn 50, Issue 5, 1998, Pages 501-507

  Hoshi, Reiun ^a  

^a RIKKYO UNIVERSITY   (Japan)

Author keywords

Accretion; Stars: individual (RX J0925.7 4758); Stars: white dwarfs; X rays: sources

Indexed keywords

HYDROGEN; WHITE DWARFS; X RAY APPARATUS;

ACCRETION; BLACKBODY TEMPERATURES; BOLOMETRIC LUMINOSITIES; COLOR TEMPERATURES; EFFECTIVE TEMPERATURE; FISH-EYE; STAR: INDIVIDUAL (RX J0925.7 - 4758); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: WHITE DWARF; X-RAY SOURCES; SOFT-X-RAY SPECTRA; STAR: INDIVIDUAL (RX J0925.7-4758);

ELECTRON SOURCES;

EID: 0032262978     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/50.5.501     Document Type: Article

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