We present a spectroscopic analysis of HST/COS observations of three massive stars in the low metallicity dwarf galaxies IC 1613 and WLM. These stars, were previously observed with VLT/X-shooter by Tramper et al. (2011, 2014) who claimed that their mass-loss rates are higher than expected from theoretical predictions for the underlying...
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2015 (v1)Journal articleUploaded on: December 4, 2022
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October 2014 (v1)Journal article
International audience
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2009 (v1)Journal article
Astronomy and Astrophysics, 501, pp. 519-530 (2009)
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2011 (v1)Journal article
International audience
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December 9, 2010 (v1)Publication
Sulfur is important: the site of its formation is uncertain, and at very low metallicity the trend of [S/Fe] against [Fe/H] is controversial. Below [Fe/H]=-2.0, [S/Fe] remains constant or it decreases with [Fe/H], depending on the author and the multiplet used in the analysis. Moreover, although sulfur is not significantly bound in dust grains...
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2011 (v1)Journal article
International audience
Uploaded on: December 3, 2022