δ centauri: A new binary Be star detected by VLTI/AMBER spectro-interferometry

Astronomy and Astrophysics

Volumn 488, Issue 3, 2008, Pages

  Meilland, A ^a   Millour, F ^a   Stee, Ph ^b   Spang, A ^b   Petrov, R ^b   Bonneau, D ^b   Perraut, K ^c   Massi, F ^d  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^c CNRS   (France)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Stars: binaries: close; Stars: circumstellar matter; Stars: emission line, Be; Stars: winds, outflows; Techniques: high angular resolution; Techniques: interferometric

Indexed keywords

FREQUENCY BANDS; GEODETIC SATELLITES; INTERFEROMETRY; SEPARATION;

BINARY SEPARATION; CIRCUMSTELLAR; ENVELOPE SIZE; LONG-BASELINE INTERFEROMETRY; SPATIAL FREQUENCIES; SPECTRAL ENERGY DISTRIBUTION; SPECTRAL-RESOLUTION; SPHERICAL SYMMETRY; STARS: BINARIES: CLOSE; STARS: CIRCUMSTELLAR MATTER; STARS: EMISSION-LINE, BE; STARS: WINDS, OUTFLOWS; TECHNIQUES: HIGH ANGULAR RESOLUTION; TECHNIQUES: INTERFEROMETRIC; TOTAL FLUX;

INTERFEROMETERS;

EID: 51949111684     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810624     Document Type: Article

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