The relationship between γ Cassiopeiae's X-ray emission and its circumstellar environment: II. Geometry and kinematics of the disk from MIRC and VEGA instruments on the CHARA Array

Astronomy and Astrophysics

Volumn 545, Issue , 2012, Pages

  Stee, P ^a   Delaa, O ^a   Monnier, J D ^c   Meilland, A ^a   Perraut, K ^b   Mourard, D ^a   Che, X ^c   Schaefer, G H ^h   Pedretti, E ⁿ   Smith, M A ^d   Lopes De Oliveira, R ^e   Motch, C ^f   Henry, G W ^g   Richardson, N D ^h   Bjorkman, K S ⁱ   Bucke R ^j   Pollmann, E ^k   Zorec, J ^m   Gies, D R ^h   Ten Brummelaar, T ^h   McAlister, H A ^h   Turner, N H ^h   Sturmann, J ^h   Sturmann, L ^h   Ridgway, S T ^l   more..

^a UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c UNIVERSITY OF MICHIGAN   (United States)

^d CATHOLIC UNIVERSITY OF AMERICA   (United States)

^e FEDERAL UNIVERSITY OF SERGIPE   (Brazil)

^f UNIVERSITÉ DE STRASBOURG   (France)

^g TENNESSEE STATE UNIVERSITY   (United States)

^h GEORGIA STATE UNIVERSITY   (United States)

ⁱ UNIVERSITY OF TOLEDO   (United States)

^j National Optical Astronomical Observatory ^*  (Germany)

^k Institut d'Astrophysique de Paris ^*  (Germany)

^l NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^m SORBONNE UNIVERSITÉ   (France)

ⁿ UNIVERSITY OF ST ANDREWS   (United Kingdom)

more..

Author keywords

Binaries: close; Circumstellar matter; Stars: emission line, Be; Stars: winds, outflows; Techniques: interferometric

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GAMMA RAYS; GEOMETRY; INFRARED DEVICES; KINEMATICS; X RAY SCATTERING; X RAYS;

BINARIES: CLOSE; CIRCUMSTELLAR MATTERS; STARS: EMISSION-LINE , BE; STARS: WINDS , OUTFLOWS; TECHNIQUES: INTERFEROMETRIC;

STARS;

EID: 84866131670     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219234     Document Type: Article

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