Stellar evolution and the 'O-rich AGB sequence'

Details Stellar evolution and the 'O-rich AGB sequence' Stellar evolution and the 'O-rich AGB sequence'

2005-08-12

arxiv.org/abs/astro-ph/0508283v1

Astronomy and Astrophysics

Astrophysics

To appear in: Proceedings of the "Stellar end products" workshop, 13-15 April 2005, Granada, Spain, ed. M.A. Perez-Torres. MmS

Scientific paper

The `O-rich AGB sequence' is a well defined area occupied by oxygen-rich AGB
stars (OH/IR) in the IRAS two-colour diagram [12]-[25] vs [25]-[60]. This
sequence is interpreted in terms of evolutionary stage and/or progenitor mass
with the aim to link observed classes of AGB stars and Planetary Nebulae (PNe).

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