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A&A 409, 205-215 (2003)
DOI: 10.1051/0004-6361:20031070
Research Note
A three-dimensional Galactic extinction model
R. Drimmel1, A. Cabrera-Lavers2 and M. López-Corredoira31 Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Torino, 10025 Pino Torinese, Italy
2 Instituto de Astrofisica de Canarias, 38200 La Laguna, Tenerife, Spain
3 Astronomisches Institut der Universität Basel, Venusstrasse 7, 4102 Binningen, Switzerland
(Received 2 May 2003 / Accepted 2 July 2003 )
Abstract
A large-scale three-dimensional model of Galactic extinction
is presented based on
the Galactic dust distribution model of Drimmel & Spergel (2001). The
extinction
AV to any point within the Galactic disk can be quickly
deduced using a set of three-dimensional Cartesian grids. Extinctions
from the model are compared to empirical extinction measures, including
lines-of-sight in and near
the Galactic plane using optical and NIR extinction
measures; in particular we show how extinction can be derived from NIR
color-magnitude diagrams in the Galactic plane to a distance of 8 kiloparsec.
Key words: dust, extinction -- ISM: structure -- Galaxy: structure
Offprint request: R. Drimmel, drimmel@to.astro.it
SIMBAD Objects
© ESO 2003
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