期刊
ASTRONOMY & ASTROPHYSICS
卷 488, 期 3, 页码 L67-L70出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:200810624
关键词
techniques : high angular resolution; techniques : interferometric; stars : emission-line, Be; stars : binaries : close; stars : winds, outflows; stars : circumstellar matter
资金
- Programme National de Physique Stellaire (PNPS)
- Institut National en Sciences de l'Univers (INSU)
- Max Planck Institut fur Radioastronomy (MPIfr)
Aims. We study the Be star delta Cen circumstellar disk using long-baseline interferometry which is the only observing technique capable of resolving spatially and spectroscopically objects smaller than 5 mas in the H and K band. Methods. We used the VLTI/AMBER instrument on January 6, 8, and 9, 2008, in the H and K bands to complete low (35) and medium (1500) spectral resolution observations. Results. We detected an oscillation in the visibility curve plotted as a function of the spatial frequency which is a clear signature of a companion around delta Cen. Our best-fit soltution infers a binary separation of 68.7 mas, a companion flux contribution in the K band of about 7% of the total flux, a PA of 117.5 degrees, and an envelope flux around the Be primary that contributes up to about 50% of the total flux, in agreement with our Spectral Energy Distribution (SED) fit. The envelope size is estimated to be 1.6 mas in K but no departure from spherical symmetry is detected.
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