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GAIA: AGB Stars as Tracers of Star Formation Histories in the Galaxy and Beyond

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Mass-Losing Pulsating Stars and their Circumstellar Matter

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 283))

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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

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3968-0

  • Online ISBN: 978-94-010-0139-7

  • eBook Packages: Springer Book Archive

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