Very luminous carbon stars in the outer disk of the Triangulum spiral galaxy
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Block, D L; Freeman, Kenneth; Jarrett, Thomas H; Puerari, I; Worthey, G; Combes, F; Groess, R
Description
Stars with masses in the range from about 1.3 to 3.5 M⊙ pass through an evolutionary stage where they become carbon stars. In this stage, which lasts a few Myr, these stars are extremely luminous pulsating giants. They are so luminous in the near-infrar
Collections | ANU Research Publications |
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Date published: | 2004 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/80342 |
Source: | Astronomy and Astrophysics |
DOI: | 10.1051/0004-6361:200400031 |
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