0000000000595062

AUTHOR

Karl-heinz Hofmann

showing 1 related works from this author

Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen

2017

Context. The star V766 Cen (=HR 5171A) was originally classified as a yellow hypergiant but lately found to more likely be a 27-36 M red supergiant (RSG). Recent observations indicated a close eclipsing companion in the contact or common-envelope phase. Aims. Here, we aim at imaging observations of V766 Cen to confirm the presence of the close companion. Methods. We used near-infrared H-band aperture synthesis imaging at three epochs in 2014, 2016, and 2017, employing the PIONIER instrument at the Very Large Telescope Interferometer (VLTI). Results. The visibility data indicate a mean Rosseland angular diameter of 4.1 ± 0.8 mas, corresponding to a radius of 1575 ± 400 R. The data show an ex…

Stars: imagingAperture synthesisBinaries: eclipsingFOS: Physical sciencesAstrophysics01 natural sciences010309 opticsCommon envelopeBinaries: closeAngular diameter0103 physical sciencesmassive [Stars]Red supergiantStars: massiveYellow hypergiant010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsVery Large Telescopeeclipsing [Binaries]Astronomy and AstrophysicsRadiusAstrophysics - Solar and Stellar AstrophysicsSupergiantsSpace and Planetary Scienceimaging [Stars]Techniques: interferometricinterferometric [Techniques]Supergiantclose [Binaries]Astronomy & Astrophysics
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