|
Volumn 353, Issue 3, 2004, Pages 841-852
|
Massive planets in FU Orionis discs: Implications for thermal instability models
|
Author keywords
Accretion, accretion discs; Instabilities; Stars: formation; Stars: pre main sequence; Stars: variables: other
|
Indexed keywords
LUMINANCE;
PLANETS;
STARS;
ACCRETION: ACCRETION DISKS;
INSTABILITY MODEL;
RISETIMES;
STAR: VARIABLE: OTHER;
STARS FORMATION;
STARS: PRE-MAIN SEQUENCE;
STARS: VARIABLES;
THERMAL INSTABILITIES;
TIME-SCALES;
YOUNG STELLAR OBJECTS;
THERMODYNAMIC STABILITY;
|
EID: 4744340496
PISSN: 00358711
EISSN: None
Source Type: Journal
DOI: 10.1111/j.1365-2966.2004.08112.x Document Type: Article |
Times cited : (172)
|
References (40)
|