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Deep Studies of the Resolved Stellar Populations in the Outskirts Of M31

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 274))

Abstract

We discuss the first results from ongoing studies of the resolved stellar populations in the outskirts of our nearest large neighbor, M31. Deep HST/WFPC2 archival observations are used to construct color-magnitude-diagrams which reach well below the horizontal branch at selected locations in the outer disk and halo, while a panoramic ground-based imaging survey maps spatial density variations through resolved star counts to a projected radius of ~ 50kpc.

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© 2002 Springer Science+Business Media Dordrecht

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Ferguson, A.M.N. (2002). Deep Studies of the Resolved Stellar Populations in the Outskirts Of M31. In: Chávez, M., Bressan, A., Buzzoni, A., Mayya, D. (eds) New Quests in Stellar Astrophysics: The Link Between Stars and Cosmology. Astrophysics and Space Science Library, vol 274. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0393-3_25

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  • DOI: https://doi.org/10.1007/978-94-010-0393-3_25

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3916-1

  • Online ISBN: 978-94-010-0393-3

  • eBook Packages: Springer Book Archive

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