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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

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Date

2009

Authors

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

Journal Title

Journal ISSN

Volume Title

Publisher

Springer

Abstract

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,

Description

Keywords

Keywords: Absolute luminosity; Abundance analysis; Borealis; Broad bands; Carbon rich; Carbon stars; Circumstellar; Colour-magnitude diagrams; Light curves; Magellanic Clouds; Midinfrared; Optical spectroscopy; Post-AGB; Shell temperatures; Spectral energy distribu Magellanic Clouds; Stars: AGB and post-AGB; Stars: carbon; Supergiants

Citation

URI

http://hdl.handle.net/1885/31776

Collections

ANU Research Publications

Source

Astronomy and Astrophysics

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1051/0004-6361/200911808

Restricted until

2037-12-31

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Description
01_Tisserand_New_Magellanic_Cloud_R_Coronae_2009.pdf (2.5 MB)

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