We present the results of a photometric survey for Be stars in 11 young clusters in the Large Magellanic Cloud and 14 young clusters in the Small Magellanic Cloud. B stars with hydrogen in emission are identified on the basis of their R-Hα colour. We fi
We present photometry in an area of 205 $\times$ 205 centered on LH 95 situated to the north-east o...
International audienceAims:We search for the effects of metallicity on B and Be stars in the Small a...
International audienceWe investigate a sample of 18 Large Magellanic Cloud Herbig Ae/Be candidate st...
We present the results of a search for Be stars in six fields centered on the young clusters NGC 330...
Recently the OGLE experiment has provided accurate light curves and colours for about 2 millions sta...
We revisited the young Large Magellanic Cloud star cluster NGC 1971 with the aim of providing additi...
Context.Detailed studies of Be stars in environments with different metallicities like the Magellani...
Observations of hot stars belonging to the young cluster LMC-NGC2004 and its surrounding region have...
Observations of hot stars belonging to the young cluster LMC-NGC 2004 and its surrounding region hav...
As part of an ongoing photometric survey of young Magellanic Cloud clusters we identified Be stars i...
talk at IAUS256At low metallicity, B-type stars show lower loss of mass and, therefore, angular mome...
Long time surveys yield many light curves among their byproducts, useful to identify candidate Be st...
Thanks to observations at the ESO VLT with the GIRAFFE multifibers spectrograph, we have obtained sp...
We revisited the young Large Magellanic Cloud star cluster NGC 1971 with the aim of providing additi...
International audienceAims.To statistically study the effects of the metallicity, star-formation con...
We present photometry in an area of 205 $\times$ 205 centered on LH 95 situated to the north-east o...
International audienceAims:We search for the effects of metallicity on B and Be stars in the Small a...
International audienceWe investigate a sample of 18 Large Magellanic Cloud Herbig Ae/Be candidate st...
We present the results of a search for Be stars in six fields centered on the young clusters NGC 330...
Recently the OGLE experiment has provided accurate light curves and colours for about 2 millions sta...
We revisited the young Large Magellanic Cloud star cluster NGC 1971 with the aim of providing additi...
Context.Detailed studies of Be stars in environments with different metallicities like the Magellani...
Observations of hot stars belonging to the young cluster LMC-NGC2004 and its surrounding region have...
Observations of hot stars belonging to the young cluster LMC-NGC 2004 and its surrounding region hav...
As part of an ongoing photometric survey of young Magellanic Cloud clusters we identified Be stars i...
talk at IAUS256At low metallicity, B-type stars show lower loss of mass and, therefore, angular mome...
Long time surveys yield many light curves among their byproducts, useful to identify candidate Be st...
Thanks to observations at the ESO VLT with the GIRAFFE multifibers spectrograph, we have obtained sp...
We revisited the young Large Magellanic Cloud star cluster NGC 1971 with the aim of providing additi...
International audienceAims.To statistically study the effects of the metallicity, star-formation con...
We present photometry in an area of 205 $\times$ 205 centered on LH 95 situated to the north-east o...
International audienceAims:We search for the effects of metallicity on B and Be stars in the Small a...
International audienceWe investigate a sample of 18 Large Magellanic Cloud Herbig Ae/Be candidate st...
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