Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-07-19
Astronomy and Astrophysics
Astrophysics
3 pages, to appear in "A Massive Star Odyssey: from Main Sequence to Supernova", ed. K. A. van der Hucht, Proc. IAU Symp. 212
Scientific paper
10.1051/0004-6361:20021569
Most of the Milky Way's evolved massive stellar population is hidden from view. We can attempt to remedy this situation with near-infrared observations, and in this paper we present our method for detecting Wolf-Rayet stars in highly extincted regions and apply it to the inner Galaxy. Using narrow band filters at K-band wavelengths, we demonstrate how WR stars can be detected in regions where they are optically obscured. Candidates are selected for spectroscopic follow-up from our relative line and continuum photometry. The final results of applying this method with a NIR survey in the Galactic plane will provide a more complete knowledge of the structure of the galactic disk, the role of metallicity in massive stellar evolution, and environments of massive star formation. In this paper we briefly describe the survey set-up and report on recent progress. We have discovered four emission-line objects in the inner Galaxy: two with nebular emission lines, and two new WR stars, both of late WC subtype.
Blum Robert
Conti Peter
Damineli Augusto
Homeier Nicole
Pasquali Anna
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