Skip navigation
Skip navigation

New Magellanic Cloud R Coronae Borealis and DY Persei type stars from the EROS-2 database: The connection between RCBs, DYPers, and ordinary carbon stars

Tisserand, Patrick; Wood, Peter R; Marquette, J B; Afonso, C; Albert, J.N.; Anderson, J; Ansari, R; Aubourg, E; Bareyre, P; Beaulieu, J.-P; Charlot, X; Coutures, C; Ferlet, R

Description

Context. R Coronae Borealis stars (RCB) are a rare type of evolved carbon-rich supergiant stars that are increasingly thought to result from the merger of two white dwarfs, called the Double degenerate scenario. This scenario is also studied as a source,

CollectionsANU Research Publications
Date published: 2009
Type: Journal article
URI: http://hdl.handle.net/1885/31776
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/200911808

Download

File Description SizeFormat Image
01_Tisserand_New_Magellanic_Cloud_R_Coronae_2009.pdf2.56 MBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator