Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-17T21:24:37.558Z Has data issue: false hasContentIssue false
  • English
  • Français

1.14. Stellar sources in a field at l ≃ −45°, B ≃ 0° of the ISOGAL survey (ISOCAM 7 and 15 microns observations)

Published online by Cambridge University Press:  25 May 2016

D.K. Ojha ,
A. Omont  and
G. Simon
D.K. Ojha
Affiliation:
T.I.F.R., Homi Bhabha Road, Colaba, Mumbai 400 005, India
A. Omont
Affiliation:
IAP, 98Bis, Bd. Arago, F-75014 Paris, France
G. Simon
Affiliation:
Observatoire de Paris, F-75014 Paris, France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

ISOGAL is a survey at 15 and 7 μm with ISOCAM of the inner Galactic disk. The survey covers ∼ 18 deg2 in selected areas of the central l = ±30 deg of the Galactic plane, all complemented by 0.8-2.2 μm DENIS data. Combined with the near infrared IJK data of the DENIS survey, it is mainly aimed at the study of the cold stellar populations of the most obscured regions of the inner Galaxy and the corresponding Galactic structure.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 43 - 44
Copyright
Copyright © Kluwer 1998 

References

Perault, M., Omont, A., Simon, G., Séguin, P., Ojha, D., et al, 1996, A&A 315, 165L.Google Scholar
Strom, K.M., Newton, G., Strom, S.E., et al., 1989, ApJS 71, 183.Google Scholar