Cyclic variability of the circumstellar disk of the Be star χ Tauri

Astronomy and Astrophysics

Volumn 504, Issue 3, 2009, Pages 915-927

  Carciofi, A C ^a   Okazaki, A T ^b   Le Bouquin, J B ^c   Stefl S ^c   Rivinius, Th ^c   Baade, D ^d   Bjorkman, J E ^e   Hummel, C A ^d  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b HOKKAI GAKUEN UNIVERSITY   (Japan)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e UNIVERSITY OF TOLEDO   (United States)

Author keywords

Methods: numerical; Polarization; Stars: emission line, Be; Stars: individual: Tauri; Techniques: interferometric

Indexed keywords

BE STARS; CIRCUMSTELLAR DISKS; CYCLIC VARIABILITIES; DISK MODEL; EMISSION LINES; METHODS: NUMERICAL; OSCILLATION MODELS; OSCILLATION PATTERNS; QUANTITATIVE TESTS; QUASI-CYCLIC; RADIATIVE TRANSFER CALCULATIONS; RADIATIVE TRANSFER CODES; RED EMISSIONS; RIGOROUS SOLUTION; SELF-CONSISTENT MODEL; SPATIALLY RESOLVED; STARS: EMISSION-LINE, BE; TECHNIQUES: INTERFEROMETRIC;

INTERFEROMETRY; NUMERICAL METHODS; POLARIZATION; RADIATIVE TRANSFER; STARS;

DISKS (STRUCTURAL COMPONENTS);

EID: 70349479889     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810962     Document Type: Article

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