Abstract
We discuss the tracing of star formation histories with ESA’s space astrometry mission GAIA, emphasizing the advantages of AGB stars for the purpose. GAIA’s microarcsecond-level astrometry, multi-band photometry and spectroscopy will provide individual distances, motions, T eff, log g and [M/H] for vast numbers of AGB stars in the Galaxy and beyond. Reliable ages of AGB stars can be determined to distances of ~200 kpc in a wide range of ages and metallicities, allowing star formation histories to be studied in a diversity of astrophysical environments
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© 2003 Springer Science+Business Media Dordrecht
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Kučinskas, A., Lindegren, L., Tanabé, T., Vansevičius, V. (2003). GAIA: AGB Stars as Tracers of Star Formation Histories in the Galaxy and Beyond. In: Nakada, Y., Honma, M., Seki, M. (eds) Mass-Losing Pulsating Stars and their Circumstellar Matter. Astrophysics and Space Science Library, vol 283. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0139-7_6
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DOI: https://doi.org/10.1007/978-94-010-0139-7_6
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