Extinction ratios in the inner Galaxy as revealed by the VVV survey
arXiv:1710.04854 · doi:10.3847/2041-8213/aa92c3
Abstract
Interstellar extinction towards the Galactic Center is large and significantly differential. Its reddening and dimming effects in red clump stars in the Galactic Bulge can be exploited to better constrain the extinction law towards the innermost Galaxy. By virtue of a deep and complete catalog of more than 30 million objets at and obtained from VVV survey observations, we apply the red clump method to infer the selective-to-total extinction ratios in the , , , and broadband near-infrared filters. The measured values are smaller than previously reported, and are not constant, with mean values, e.g., and . We also obtain a ratio :::: of 7.74:5.38:3.30:1.88:1.0, implying extinction towards the Galactic Center to follow a distribution as a function of wavelength steeper than previously reported, consistent with a power law in the near-infrared.
Accepted for publication in ApJ Letters, 10 pages, 3 Figures, 2 Tables
References in corpus (2)
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