AGB stars in the Local Group, and beyond

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I summarize the current status of surveys for late-type M, and Carbon stars in the Local Group based on three different approaches that make use of the characteristics of these stars: spectral characteristics using narrow-band filters, infrared characteristics, and variability.
Invited review at the conference: "Planetary Nebulae beyond the Milky Way". Presentation is available at: http://www.ster.kuleuven.ac.be/~groen/presentation.html

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/7949

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0407282
 http://arxiv.org/abs/astro-ph/0407282

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arXiv