The Mira variable S Orionis: Relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs

Astronomy and Astrophysics

Volumn 470, Issue 1, 2007, Pages 191-210

  Wittkowski, M ^a   Boboltz, D A ^b   Ohnaka, K ^c   Driebe, T ^c   Scholz, M ^d,e  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b US NAVAL OBSERVATORY   (United States)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^d UNIVERSITY OF HEIDELBERG   (Germany)

^e UNIVERSITY OF SYDNEY   (Australia)

Author keywords

Masers; Stars: AGB and post AGB; Stars: atmospheres; Stars: individual: S Orionis; Stars: mass loss; Techniques: interferometric

Indexed keywords

DATA ACQUISITION; DYNAMIC MODELS; INTERFEROMETRY; KINEMATICS; MASERS; OXYGEN; STARS;

STARS: AGB AND POST-AGB; STARS: ATMOSPHERES; STARS: INDIVIDUAL: S ORIONIS; STARS: MASS-LOSS;

ASTROPHYSICS;

EID: 34547197872     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077168     Document Type: Article

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