THE KEPLER LIGHT CURVE OF V344 Lyrae: CONSTRAINING THE THERMAL-VISCOUS LIMIT CYCLE INSTABILITY

Record Type
Journal Articles
Full Title
THE KEPLER LIGHT CURVE OF V344 Lyrae: CONSTRAINING THE THERMAL-VISCOUS LIMIT CYCLE INSTABILITY
Author(s)
Cannizzo J, Still M, Howell S, Wood M, Smale A
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2010 Dec
DOI
10.1088/0004-637X/725/2/1393
ISSN
0004-637X
Volume
725
Issue
2
Page Count
12
First Page
1393
Last Page
1404
Keyword(s)
Astronomy & Astrophysics, novae, cataclysmic variables, stars: dwarf novae, stars: individual (V344 Lyr), white dwarfs, DWARF-NOVA OUTBURSTS, ENHANCED MASS-TRANSFER, SU UMA-TYPE, PARTICLE HYDRODYNAMICS SIMULATIONS, CLOSE BINARY-SYSTEMS, URSAE MAJORIS STARS, ACCRETION DISKS, SS-CYGNI, CATACLYSMIC VARIABLES, X-RAY
Citation
Cannizzo J, Still M, Howell S, Wood M, Smale A. THE KEPLER LIGHT CURVE OF V344 Lyrae: CONSTRAINING THE THERMAL-VISCOUS LIMIT CYCLE INSTABILITY. ASTROPHYS J. 2010;725 (2):1393-1404.
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