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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 230))

Abstract

ISOGAL is the first near+mid-infrared, high-resolution imaging survey of the inner disk and bulge of the Milky Way Galaxy (Pérault et al. 1996). The ISO satellite, and especially ISOCAM, allows a quantum jump in observational analyses of Galactic structure and stellar populations, star formation and infrared properties of the interstellar medium, especially in the most obscured regions of the inner Galactic disk. The combination of ISOCAM data with DENIS (Epchtein et al. 1997) IJK data allows characterisation of the stellar populations.

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© 1998 Springer Science+Business Media Dordrecht

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Omont, A. et al. (1998). Mass-Losing AGB Stars and Young Stars in the Isogal Survey. In: Epchtein, N. (eds) The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy. Astrophysics and Space Science Library, vol 230. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5026-2_6

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  • DOI: https://doi.org/10.1007/978-94-011-5026-2_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6110-0

  • Online ISBN: 978-94-011-5026-2

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