Long-term monitoring of θ1 Ori C: The spectroscopic orbit and an improved rotational period

Astronomy and Astrophysics

Volumn 487, Issue 1, 2008, Pages 323-327

  Stahl, O ^a   Wade, G ^b   Petit, V ^c   Stober, B ^d   Schanne, L ^d  

^a UNIVERSITÄT HEIDELBERG   (Germany)

^b ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^c UNIVERSITÉ LAVAL   (Canada)

^d NONE   (Germany)

Author keywords

Stars: circumstellar matter; Stars: early type; Stars: emission line, Be; Stars: individual: 1 Ori C; Stars: variables: general

Indexed keywords

EQUIVALENT WIDTH; LONG TERM TRENDS; LONG-TERM MONITORING (LTM); MAGNETIC (CE); RADIAL VELOCITY (RV); SPECTRA (CO); SPECTROSCOPIC DATA; VARIATIONS OF;

STARS;

EID: 48249156629     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809935     Document Type: Article

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