Kinematics and geometrical study of the Be stars 48 Persei and ψ Persei with the VEGA/CHARA interferometer

Astronomy and Astrophysics

Volumn 529, Issue , 2011, Pages

  Delaa, O ^a,c   Stee, Ph ^a   Meilland, A ^b   Zorec, J ^c   Mourard, D ^a   Berio Ph ^a   Bonneau, D ^a   Chesneau, O ^a   Clausse, J M ^a   Cruzalebes, P ^a   Perraut, K ^d   Marcotto, A ^a   Roussel, A ^a   Spang, A ^a   McAlister, H ^e,f   Ten Brummelaar, T ^f   Sturmann, J ^f   Sturmann, L ^f   Turner, N ^f   Farrington, C ^f   Goldfinger, P J ^f   more..

^a UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^d UNIV GRENOBLE ALPES   (France)

^e GEORGIA STATE UNIVERSITY   (United States)

^f Mount Wilson Observatory   (United States)

Author keywords

Circumstellar matter; Stars: emission line, Be; Stars: individual: 48 Per; Stars: individual: Per; Stars: winds, outflows; Techniques: interferometric

Indexed keywords

CIRCUMSTELLAR MATTERS; STARS: EMISSION-LINE, BE; STARS: INDIVIDUAL: 48 PER; STARS: WINDS, OUTFLOWS; TECHNIQUES: INTERFEROMETRIC;

INCOHERENT SCATTERING; INTERFEROMETERS; INTERFEROMETRY; KINEMATICS; MAGNETIC FIELDS; ROTATION; WIND;

STARS;

EID: 79953779823     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015639     Document Type: Article

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