AGB stars in the Local Group, and beyond

2004/07/14 by M. A. T. Groenewegen, Martin Groenewegen, Groenewegen, Martin
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0407282

Invited review at the conference: "Planetary Nebulae beyond the Milky Way". Presentation is available at: http://www.ster.kuleuven.ac.be/~groen/presentation.html

arxiv created 2004/07/14 · openalex publication_date 2004/07/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

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.

Related

• Populations of AGB stars and LPVs in the Galaxy and Local Group
• AGB star in the Magellanic Clouds & in other members of the Local Group
• AGB stars and the plate archives heritage
• AGB candidates in the field of gamma Cas
• Carbon stars in the Local Group