A large H α line forming region for the massive interacting binaries β Lyrae and υ Sagitarii

Astronomy and Astrophysics

Volumn 532, Issue , 2011, Pages

  Bonneau, D ^a   Chesneau, O ^a   Mourard, D ^a   Bério, Ph ^a   Clausse, J M ^a   Delaa, O ^a   Marcotto, A ^a   Perraut, K ^b   Roussel, A ^a   Spang, A ^a   Stee, Ph ^a   Tallon Bosc, I ^c   McAlister, H ^d,e   Ten Brummelaar, T ^e   Sturmann, J ^e   Sturmann, L ^e   Turner, N ^e   Farrington, C ^e   Goldfinger, P J ^e  

^a UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c UNIVERSITÉ LYON 1   (France)

^d GEORGIA STATE UNIVERSITY   (United States)

^e Mount Wilson Observatory   (United States)

Author keywords

Binaries: close; Circumstellar matter; Stars: emission line, Be; Stars: individual: Lyrae; Stars: individual: Sagittarii; Stars: mass loss

Indexed keywords

BINARIES: CLOSE; CIRCUMSTELLAR MATTERS; STARS: EMISSION-LINE, BE; STARS: INDIVIDUAL; STARS: MASS-LOSS;

ELECTROMAGNETIC WAVE EMISSION; INTERFEROMETRY; VISIBILITY;

STARS;

EID: 80051495102     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116742     Document Type: Article

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