Spiral structure in IP Pegasi: How persistent is it?

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 3, 2000, Pages 454-460

  Morales Rueda, L ^a   Marsh, T R ^a   Billington, I ^b  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b Swiss Bank Corporation   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: Spectroscopic; Line: Profiles; Novae, cataclysmic variables; Stars: Individual: IP Peg; Stars: Mass loss

Indexed keywords

EXTREME ULTRAVIOLET LITHOGRAPHY; MAGNESIUM COMPOUNDS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES: SPECTROSCOPIC; LINE: PROFILES; NOVAE CATACLYSMIC VARIABLES; PEGASIS; PEGASUS; SPIRAL STRUCTURES; STARS: MASS-LOSS; STARS:INDIVIDUAL:IP PEG;

STARS;

EID: 0000788640     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03330.x     Document Type: Article

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