Estrellas Wolf-Rayet de tipo WN en La Vía Láctea: Campaña 2007-2008

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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4 pages, 2 figures, full text in Spanish, accepted for BAAA

Scientific paper

We are carrying out a spectroscopic monitoring of Galactic Wolf-Rayet stars,
in order to detect binary systems. The sample consists of approximately 50
stars of the Nitrogen sequence (WN) and fainter than V = 13. The observations
are made from the 4-m telescope at CTIO, Chile. In the following, we present
the first results of the 2007-2008 campaign.

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