Non-local thermal equilibrium model atmospheres for the hottest white dwarfs: Spectral analysis of the compact component in nova V4743Sgr

Astrophysical Journal

Volumn 717, Issue 1, 2010, Pages 363-371

  Rauch, T ^a   Orio, M ^b,c   Gonzales Riestra, R ^d   Nelson, T ^e,f   Still, M ^g,h   Werner, K ^a   Wilms, J ⁱ  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^c UNIVERSITY OF WISCONSIN MADISON   (United States)

^d EUROPEAN SPACE AGENCY   (Spain)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^g NASA AMES RESEARCH CENTER   (United States)

^h UNIVERSITY COLLEGE LONDON   (United Kingdom)

ⁱ UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

Author keywords

Cataclysmic variables; Novae; Stars: abundances; Stars: AGB and post AGB; Stars: atmospheres; Stars: individual (V4743 Sgr); White dwarfs

Indexed keywords

EID: 77953741157     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/717/1/363     Document Type: Article

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