0000000000595064

AUTHOR

J. Sanchez-bermudez

showing 2 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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A VLBI study of the wind-wind collision region in the massive multiple HD 167971

2019

Context. Colliding winds in massive binaries are able to accelerate particles up to relativistic speeds as the result of the interaction between the winds of the different stellar components. HD 167971 exhibits this phenomenon which makes it a strong radio source. Aims. We aim at characterizing the morphology of the radio emission and its dependence on the orbital motion, traced independently by near-infrared (NIR) interferometry of both the spectroscopic binary and the tertiary component comprising HD 167971. Methods. We analyze 2006 and 2016 very long baseline interferometric data at C and X bands. We complement our analysis with a geometrical model of the wind-wind collision region and a…

Radiation mechanisms: non-thermalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesTechniques: high angular resolutionMomentum0103 physical sciencesVery-long-baseline interferometryBinaries: generalmassive [Stars]Astrophysics::Solar and Stellar AstrophysicsStars: mass-lossStars: massive010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsSpectral indexmass-loss [Stars]non-thermal [Radiation mechanisms]general [Binaries]010308 nuclear & particles physicsComputer Science::Information RetrievalAstronomy and AstrophysicsCollisionhigh angular resolution [Techniques]StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTechniques: interferometricPhysics::Space PhysicsOrbital motioninterferometric [Techniques]Astronomy & Astrophysics
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