The extreme T Tauri star RW Aur: Accretion and outflow variability

Astronomy and Astrophysics

Volumn 440, Issue 2, 2005, Pages 595-608

  Alencar, S H P ^a,d   Basri, G ^b   Hartmann, L ^c   Calvet, N ^c  

^a FEDERAL UNIVERSITY OF MINAS GERAIS   (Brazil)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIV GRENOBLE ALPES   (France)

Author keywords

Stars: pre main sequence; Line: profiles; Stars: formation; Stars: individual: RW Aur; Stars: winds, outflows

Indexed keywords

LIGHT EMISSION; MAGNETIC FIELD EFFECTS; MAGNETOSPHERE; WIND;

LINE: PROFILES; STARS: FORMATION; STARS: INDIVIDUAL: RW AUR; STARS: PRE-MAIN SEQUENCE; STARS: WINDS, OUTFLOWS;

ASTROPHYSICS;

EID: 24944447830     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053315     Document Type: Article

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