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Near Infrared Survey of the Nuclear Regions of the Milky Way

Published online by Cambridge University Press:  01 August 2006

U. C. Joshi ,
S. Ganesh ,
K. S. Baliyan ,
I. S. Glass  and
T. Nagata
U. C. Joshi
Affiliation:
Physical Research Laboratory, India
S. Ganesh
Affiliation:
Physical Research Laboratory, India
K. S. Baliyan
Affiliation:
Physical Research Laboratory, India
I. S. Glass
Affiliation:
South African Astronomical Observatory, South Africa
T. Nagata
Affiliation:
Nagoya University, Japan
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Abstract

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Results based on the deep imaging survey of the inner region (~300pc of the bulge within |ℓ| ~ 1.5°, |b| ~ 0.5°) of the Milky Way are reported in this communication. This survey is about 2.5 magnitude deeper than DENIS and 2MASS and is able to detect stars of the red clump at a distance of the Galactic center. Toward some directions we find extinction reaching AV = 50 mag. A catalog of the sources is in preparation.

Keywords

Milky-wayinterstellar extinctionGalactic Bulge
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 105 - 108
Copyright
Copyright © International Astronomical Union 2007