Emission line stars in young open clusters with ESO-WFI-spectrograph

Details Emission line stars in young open clusters with ESO-WFI-spectrograph Emission line stars in young open clusters with ESO-WFI-spectrograph

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..303m&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

-We used the ESO Wide Field Imager(WFI) in spectroscopic mode(very low resolution) in order to search and detect stars with Halpha emission line in the Large & Small Magellanic Clouds. We present our detection methods and our first results. -We used the ESO-WFI-spectro with Rc filter in order to detect new Be stars in NGC6611 and Westerlund1. We present the results of this study and compare with previous studies. -And we compare with our VLT-FLAMES studies(10/2003,04/2004).

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