Hydrodynamic Modeling of a Flare Loop Connecting the Accretion Disk and Central Core of Young Stellar Objects

Publications of the Astronomical Society of Japan

Volumn 55, Issue 5, 2003, Pages 967-980

  Isobe, Hiroaki ^a   Shibata, Kazunari ^a   Yokoyama, Takaaki ^b,c   Imanishi, Kensuke ^d  

^a KYOTO UNIVERSITY   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d KYOTO UNIVERSITY   (Japan)

Author keywords

Hydrodynamics; Stars: flare; Stars: pre main sequence; X rays: stars

Indexed keywords

STARS;

ACCRETION DISCS; CENTRAL CORE; HYDRODYNAMIC MODELING; PROTOSTARS; STARS: FLARE; STARS: PRE-MAIN SEQUENCE; SYNTHESISED; T TAURI STARS; X-RAY:STARS; YOUNG STELLAR OBJECTS;

HYDRODYNAMICS;

EID: 0346902951     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/55.5.967     Document Type: Article

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