Testing the line-driven disc wind model: Time-resolved ultraviolet spectroscopy of IX Vel and V3885 Sgr

Monthly Notices of the Royal Astronomical Society

Volumn 332, Issue 1, 2002, Pages 127-143

  Hartley, L E ^a   Drew, J E ^a   Long, K S ^b   Knigge, C ^c   Proga, D ^d,e  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b STScI   (United States)

^c UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e UNIVERSITY OF COLORADO   (United States)

Author keywords

Binaries: close; Line: profiles; Novae, cataclysmic variables; Stars: mass loss; Ultraviolet: stars

Indexed keywords

LUMINANCE; SILICON COMPOUNDS; TIME MEASUREMENT; WHITE DWARFS;

BINARIES: CLOSE; DRIVEN DISCS; LINE: PROFILES; NOVAE CATACLYSMIC VARIABLES; STARS: MASS-LOSS; TIME-SCALES; ULTRA-VIOLET SPECTRUMS; ULTRAVIOLET SPECTRUM; ULTRAVIOLET: STARS; WIND MODELLING;

ULTRAVIOLET SPECTROSCOPY;

EID: 0012665192     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05277.x     Document Type: Article

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