Title of article
Are the stellar winds in IC 1613 stronger than expected?
Author/Authors
Artemio Herrero، نويسنده , , Maria Garcia، نويسنده , , Katrien Uytterhoeven، نويسنده , , Francisco Najarro، نويسنده , , Daniel J. Lennon، نويسنده , , Sergio Simon-Diaz، نويسنده , , Norberto Castro، نويسنده , , Joachim Puls، نويسنده , , Jorick S. Vink، نويسنده , , Miguel A. Urbaneja، نويسنده , , Alex de Koter، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
2
From page
292
To page
293
Abstract
In this poster we present the results of our analyses of three early massive stars in IC 1613, whose spectra have been observed with VIMOS and analyzed with CMFGEN and FASTWIND. One of the targets resulted a possible LBV and the other two are Of stars with unexpectedly strong winds. The Of stars seem to be strongly contaminated by CNO products. Our preliminary results may represent a challenge for the theory of stellar atmospheres, but they still have to be confirmed by the analysis of more objects and a more complete coverage of the parameter space.
Keywords
stars: atmospheres , stars: early-type , galaxies: individual (IC 1613) , stars: mass loss , stars: fundamental parameters
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667867
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