The circumbinary dusty disk around the hydrogen-deficient binary star v Sagittarii

Astronomy and Astrophysics

Volumn 499, Issue 3, 2009, Pages 827-833

  Netolicky M ^a,b   Bonneau, D ^c   Chesneau, O ^c   Harmanec, R ^d   Koubsky R ^a   Mourard, D ^c   Stee, P ^c  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

^b MASARYK UNIVERSITY   (Czech Republic)

^c UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^d CHARLES UNIVERSITY   (Czech Republic)

Author keywords

Be Stars: Binaries: Close ; Stars: Circumstellar matter ; Stars: Emission line; Techniques: Interferometric stars: Individual: V sagittarii

Indexed keywords

BAND SPECTRUM; BE - STARS: BINARIES: CLOSE -; BINARY STAR; BINARY SYSTEMS; CARBON DUST; CHEMICAL COMPOSITIONS; DISK MODEL; DUST COMPOSITION; DUSTY DISKS; MIDINFRARED; ORBITAL PARAMETERS; PARAMETER SPACES; POSITION ANGLE; STARS: CIRCUMSTELLAR MATTER -; STARS: EMISSION-LINE; TECHNIQUES: INTERFEROMETRIC STARS: INDIVIDUAL: V SAGITTARII; THIN DISK;

DISKS (STRUCTURAL COMPONENTS); DUST; EMISSION SPECTROSCOPY; HYDROGEN; INTERFEROMETRY; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; ORBITAL LABORATORIES; SILICATES; SPACECRAFT OBSERVATORIES; TELESCOPES; VISIBILITY;

STARS;

EID: 66949181481     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811192     Document Type: Article

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