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Starforming region M 16: A near and mid IR study

Published online by Cambridge University Press:  25 September 2002

M. Giard ,
J.P. Bernard ,
A. Klotz ,
I. Ristorcelli ,
U. C. Joshi ,
S. Ganesh ,
K. S. Baliyan ,
G. Simon ,
A. Omont  and
M. Schultheis
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U. C. Joshi*
Affiliation:
Physical Research Laboratory, Ahmedabad, India
S. Ganesh
Affiliation:
Physical Research Laboratory, Ahmedabad, India
K. S. Baliyan
Affiliation:
Physical Research Laboratory, Ahmedabad, India
G. Simon
Affiliation:
Observatoire de Paris, Paris, France
A. Omont
Affiliation:
Institut d'Astrophysique de Paris, Paris, France
M. Schultheis
Affiliation:
Institut d'Astrophysique de Paris, Paris, France
F. Schuller
Affiliation:
Institut d'Astrophysique de Paris, Paris, France
*
joshi@prl.ernet.in
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Abstract

The Inner Region of the Galaxy has been enigmatic. Some interesting results are becoming available now from the highly promising near and mid infrared surveys such as DENIS, 2MASS, ISOGAL, of this region. The DENIS and ISOGAL surveys have already produced several interesting results over the past couple of years. We have made complementary observations towards the M 16 starforming region to provide additional data at an intermediate wavelength (H band) compared to the DENIS survey. The data will be used in combination with the other 5 bands from the ISOGAL/DENIS survey to characterise the stellar populations in this region.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 4: Infrared and Submillimeter Space Astronomy: An International Colloquium to Honor the Memory of Guy Serra , 2002 , pp. 351
Copyright
© EAS, EDP Sciences, 2002

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