Peering through the veil: near-infrared photometry and extinction for the Galactic nuclear star cluster
R. Schoedel, F. Najarro, K. Muzic, A. Eckart

TL;DR
This study provides detailed near-infrared photometry and extinction measurements for the Galactic center, revealing spatial variability and refining the extinction law and distance estimates with high precision.
Contribution
It offers the first comprehensive extinction law and high-resolution extinction maps for the central parsec of the Milky Way using adaptive optics data.
Findings
Measured absolute extinction values in H, Ks, and L'-bands.
Derived the power-law indices of the extinction law.
Produced high-resolution extinction maps of the Galactic center.
Abstract
The aims of this work are to provide accurate photometry in multiple near-infrared broadband filters, to determine the power-law index of the extinction-law toward the central parsec of the Galaxy, to provide measurements of the absolute extinction toward the Galactic center, and finally to measure the spatial variability of extinction on arcsecond scales.We use adaptive optics observations of the central parsec of the Milky Way. Absolute values for the extinction in the H, Ks, and L'-bands as well as of the power-law indices of the H to Ks and Ks to L' extinction-laws are measured based on the well-known properties of red clump stars. Extinction maps are derived based on H-Ks and Ks-L' colors. We present Ks-band photometry for ~7700 stars (H and L' photometry for a subset). From a number of recently published values we compute a mean distance of the Galactic center of R_0=8.03+-0.15…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
