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2.6. Resolved near-IR survey of the inner Galaxy
Published online by Cambridge University Press: 25 May 2016
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The analysis of resolved DENIS (Deep Near Infra Red Survey of the Southern Sky) I,J and K band data shows good evidence (≳ 3σ) in the J and K band number counts to support the existence of a kiloparsec-scale bar with its major axis in the first quadrant. A star by star dereddening of this K data combined with supplementary nbL band data (3.6μm) gives number count contrasts consistent with low angle (≲ 20 degrees) bar models in the literature.
- Type
- Part I. Stellar Cluster, Star Formation
- Information
- Copyright
- Copyright © Kluwer 1998
References
Binney, J., Gerhard, O.E., Stark, A.A., Bally, J., Uchida, K.I., 1991, MNRAS, 252, 210.Google Scholar
Matsumoto, T. et al., 1982, in The Galactic Center, AIP Conf. Proc. 83, Riegler, G.R., Blandford, R.D., eds, AIP, New York, 48.Google Scholar
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