Stellar evolution and the 'O-rich AGB sequence'

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dc.creatorJimenez-Esteban, F. M.
dc.creatorEngels, D.
dc.creatorGarcia-Lario, P.
dc.date2005-08-12
dc.date.accessioned2026-07-07T02:18:27Z
dc.date.available2026-07-07T02:18:27Z
dc.descriptionThe `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).
dc.descriptionTo appear in: Proceedings of the "Stellar end products" workshop, 13-15 April 2005, Granada, Spain, ed. M.A. Perez-Torres. MmSAI Vol. 77 (2006) (3 pages, 4 figures)
dc.identifierhttps://arxiv.org/abs/astro-ph/0508283
dc.identifierhttp://arxiv.org/abs/astro-ph/0508283
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9491
dc.subjectAstrophysics
dc.titleStellar evolution and the 'O-rich AGB sequence'
dc.typetext

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