A self-consistent optical, ultraviolet, and extreme-ultraviolet model for the spectrum of the hot white dwarf G191-B2B

Astrophysical Journal

Volumn 473, Issue 2 PART I, 1996, Pages 1089-1093

  Lanz, T ^a   Barstow, M A ^b   Hubeny, I ^a   Holberg, J B ^c  

^a UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c UNIVERSITY OF ARIZONA   (United States)

Author keywords

Stars: abundances; Stars: individual (G191 B2B); Ultraviolet: stars; White dwarfs

Indexed keywords

EID: 21444437934     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/178218     Document Type: Article

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