Abstract
We have developed a method for the determination of stellar parameters and interstellar extinction values from multicolor photometry. The application of this method to a set of stars in a small area in the sky allows us to determine an increase of interstellar extinction with distance in that direction and, consequently, to construct a 3D extinction map of the Milky Way Galaxy.
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Schedule a callMore From: Astronomical and Astrophysical Transactions, Vol. 33, No. 4
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