Volume 438, Number 1, July IV 2005
|Page(s)||169 - 185|
|Section||Interstellar and circumstellar matter|
|Published online||06 July 2005|
Optimal column density measurements from multiband near-infrared observations
European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching bei München, Germany e-mail: email@example.com
2 University of Milan, Department of Physics, via Celoria 16, 20133 Milan, Italy
Accepted: 22 March 2005
We consider from a general point of view the problem of determining the extinction in dense molecular clouds. We use a rigorous statistical approach to characterize the properties of the most widely used optical and infrared techniques, namely the star count and the color excess methods. We propose a new maximum-likelihood method that takes advantage of both star counts and star colors to provide an optimal estimate of the extinction. Detailed numerical simulations show that our method performs optimally under a wide range of conditions and, in particular, is significantly superior to the standard techniques for clouds with high column-densities and affected by contamination by foreground stars.
Key words: dust, extinction / methods: statistical / ISM: clouds / infrared: ISM / stars: formation
© ESO, 2005
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