The binary Be star δ Scorpii at high spectral and spatial resolution : I. Disk geometry and kinematics before the 2011 periastron

Astronomy and Astrophysics

Volumn 532, Issue , 2011, Pages

  Meilland, A ^a   Delaa, O ^b   Stee, Ph ^b   Kanaan, S ^c   Millour, F ^b   Mourard, D ^b   Bonneau, D ^b   Petrov, R ^b   Nardetto, N ^b   Marcotto, A ^b   Roussel, A ^b   Clausse, J M ^b   Perraut, K ^d   McAlister, H ^e,f   Ten Brummelaar, T ^f   Sturmann, J ^f   Sturmann, L ^f   Turner, N ^f   Ridgway, S T ^g   Farrington, C ^f   Goldfinger, P J ^f   more..

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c UNIVERSIDAD DE VALPARAÍSO   (Chile)

^d UNIV GRENOBLE ALPES   (France)

^e GEORGIA STATE UNIVERSITY   (United States)

^f Mount Wilson Observatory   (United States)

^g NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

Author keywords

Be; circumstellar matter; stars: emission line; stars: individual: Sco; stars: mass loss; techniques: high angular resolution; techniques: interferometric

Indexed keywords

CIRCUMSTELLAR MATTERS; STARS: EMISSION-LINE; STARS: MASS-LOSS; TECHNIQUES: HIGH ANGULAR RESOLUTIONS; TECHNIQUES: INTERFEROMETRIC;

GEOMETRY; INTERFEROMETRY; KINEMATICS; ROTATION;

STARS;

EID: 79960794490     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116798     Document Type: Article

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