Volume 462, Number 3, February II 2007
|Page(s)||965 - 976|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||13 November 2006|
The surface brightness of the Galaxy at the solar neighbourhood *
LERMA, Université Pierre et Marie Curie and Observatoire de Paris, 61 avenue de l'Observatoire, 75014 Paris, France e-mail: Anne-Laure.Melchior@obspm.fr; Francoise.Combes@obspm.fr
2 Department of Astronomy, Ohio State University, Columbus Ohio 43210, USA e-mail: email@example.com
Accepted: 2 November 2006
We present a new determination of the surface brightness of our Galaxy at the Solar Neighbourhood as observed from outside the Galaxy. We rely on various existing optical and infra-red surveys to obtain a multiwavelength estimate. On the one hand, scattered light does not contribute significantly to the surface brightness. On the other hand, optical and infrared integrated all-sky surveys (Pioneer 10/11 and COBE/DIRBE) show a systematically larger value than our synthetic local estimate based on Hipparcos data. This local estimate is also compatible with our Galactic simulations normalised at the Solar Neighbourhood and assuming a homogeneous stellar distribution. We interpret this disagreement as a signature of the presence of a local minimum of the stellar density compatible with Gould's belt. According to this result, the global luminosity of the Milky Way should follow the Tully-Fisher relation established for external galaxies.
Key words: Galaxy: solar neighbourhood / cosmology: diffuse radiation / radiation mechanisms: thermal / methods: data analysis / ISM: general
© ESO, 2007
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