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Mass-Losing AGB Stars and Young Stars in the Isogal Survey

  • A. Omont
  • B. Caillaud
  • P. Fouque
  • G. Gilmore
  • D. Ojha
  • M. Perault
  • P. Seguin
  • G. Simon
  • R. F. G. Wyse
Conference paper
Part of the Astrophysics and Space Science Library book series (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.

Keywords

Star Formation Stellar Population Young Star Galactic Disk Interstellar Extinction 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • A. Omont
    • 1
  • B. Caillaud
    • 1
  • P. Fouque
    • 2
  • G. Gilmore
    • 3
  • D. Ojha
    • 4
  • M. Perault
    • 5
  • P. Seguin
    • 5
  • G. Simon
    • 6
  • R. F. G. Wyse
    • 7
    • 8
  1. 1.Institut d’Astrophysique de Paris-CNRSFrance
  2. 2.Observatoire de Paris, DESPAFrance and European Southern ObservatoryChile
  3. 3.Institute of AstronomyCambridgeUK
  4. 4.TIFRBombayIndia
  5. 5.Laboratoire de Radioastronomie MillimétriqueENS and CNRSParisFrance
  6. 6.Observatoire de ParisDASGALFrance
  7. 7.John Hopkins UniversityBaltimoreUSA
  8. 8.THE ISOGAL-DENIS TEAMUSA

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