Infrared extinction in the Inner Milky Way through the red clump giants
arXiv:1402.0083 · doi:10.1088/0004-637X/782/2/86
Abstract
While the shape of the extinction curve on the infrared is considered to be set and the extinction ratios between infrared bands are usually taken to be approximately constant, a recent number of studies point either to a spatially variable behavior on the exponent of the power law or to a different extinction law altogether. In this paper, we propose a method to analyze the overall behavior of the interstellar extinction by means of the red-clump population, and we apply it to those areas of the Milky Way where the presence of interstellar matter is heavily felt: areas located in 5 deg<l<30 deg and b=0 deg. We show that the extinction ratios traditionally used for the near infrared could be inappropriate for the inner Galaxy and we analyze the behavior of the extinction law from 1 to 8 microns.
Accepted for publication on ApJ
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- The Optical -- Mid-infrared Extinction Law of the l=165 Sightline in the Galactic Plane: Diversity of Extinction Law in the Diffuse Interstellar Medium
- Near-infrared photometry and spectroscopy of the low Galactic latitude globular cluster 2MASS-GC03
- Time-Series Surveys and Pulsating Stars: The Near-Infrared Perspective
- Interstellar Extinction Law toward the Galactic Center IV: J, H, and Ks Bands from VVV Red Clump Stars
- Hidden power of near-infrared data for the study of young clusters: Illustrative case of RCW 38
- Variable Stars in M31 Stellar Clusters from the Panchromatic Hubble Andromeda Treasury