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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


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
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/200911808


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