The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase

Journal Article

2014

Permanent link to this Item
http://hdl.handle.net/11427/34303
Files
ChesneauO_yellow_hypergia_2014.pdf (5.37 MB)
Authors
Chesneau, O
Meilland, A
Kanaan, S
Bendjoya, Ph
Feast, M W
Groh, J H
Lobel, A
Nardetto, N
Otero, S
Oudmaijer, R D
Tekola, A G
Whitelock, P A
Chapellier, E
Arcos, C
Curé, M
Vanzi, L
Millour, F
van Genderen, A M
Nazé, Y
Smith, N
Spang, A
Smoker, J V
Dessart, L
Journal Title

Astronomy and Astrophysics

Link to Journal
https://dx.doi.org/10.1051/0004-6361/201322421
Journal ISSN
Volume Title
Publisher
Publisher
Department
Department of Astronomy
Faculty
Faculty of Science
License
Series
Abstract
Context. Only a few stars are caught in the very brief and often crucial stages when they quickly traverse the Hertzsprung-Russell diagram, and none has yet been spatially resolved in the mass transfer phase.
Description
Keywords
circumstellar matter
: Space science, astronomy
massive [stars]
Astrophysics - Solar and Stellar Astrophysics
techniques: high angular resolution
stars: individual: HR 5171 A
binaries: close
stars: massive
stars: mass
astrophysics [G05] [Physical, chemical, mathematical and earth Sciences]
mass-loss [stars]
: Aérospatiale, astronomie
astrophysique [G05] [Physique, chimie, mathématiques
sciences de la terre]
high angular resolution [techniques]
individual: HR 5171 A [stars]
close [binaries]

Reference:

Chesneau, O., Meilland, A., Chapellier, E., Millour, F., van Genderen, A.M., Nazé, Y., Smith, N. & Spang, A. et al. 2014. The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase. Astronomy and Astrophysics. 563(4):A71 - 177. http://hdl.handle.net/11427/34303

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