Proceedings IAUS266 at the IAU-GA 2009NGC6611, Trumpler 14, Trumpler 15, Trumpler 16, Collinder 232 are very young open clusters located in star-formation regions of the Eagle Nebula or the Carina in the MW, and NGC346 in the SMC. With different instrumentations and techniques, it was possible to detect and classify new Herbig Ae/Be stars, classical Be stars and to provide new tests / comparisons about the Be stars appearance models. Special stars (He-strong) of these star-formation regions are also presented
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
International audienceContext. Stellar physical properties of star clusters are poorly known and the...
Abstract. Emission-line stars in young open clusters are identified to study their properties, as a ...
Proceedings IAUS266 at the IAU-GA 2009NGC6611, Trumpler 14, Trumpler 15, Trumpler 16, Collinder 232 ...
sf2a 2006We report on the study of the population of B and Be stars in SMC young clusters, performed...
talk at IAUS256At low metallicity, B-type stars show lower loss of mass and, therefore, angular mome...
This work deals with the search of Be stars and sources with H$\alpha$ emission line in the Large an...
Emission-line stars in young open clusters are identified to study their properties, as a function o...
proceedings SF2A2008, PNPS sessionThis document presents the results from our spectroscopic survey o...
We present the spectroscopic study of 5 Herbig Ae/Be stars in young open clusters. These are identif...
We present the results of a search for Be stars in six fields centered on the young clusters NGC 330...
Proceedings corresponding to poster 581 from the Special Session 7 about young stellar objects at th...
With the Palomar Transient Factory Survey, we report Be stars candidates in the open cluster NGC 663...
AbstractWe recently launched a comprehensive ground based (ESO/VLT/NTT) and space (HST & SST) study ...
Context.By studying young open clusters, the mechanisms important for star formation over several M...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
International audienceContext. Stellar physical properties of star clusters are poorly known and the...
Abstract. Emission-line stars in young open clusters are identified to study their properties, as a ...
Proceedings IAUS266 at the IAU-GA 2009NGC6611, Trumpler 14, Trumpler 15, Trumpler 16, Collinder 232 ...
sf2a 2006We report on the study of the population of B and Be stars in SMC young clusters, performed...
talk at IAUS256At low metallicity, B-type stars show lower loss of mass and, therefore, angular mome...
This work deals with the search of Be stars and sources with H$\alpha$ emission line in the Large an...
Emission-line stars in young open clusters are identified to study their properties, as a function o...
proceedings SF2A2008, PNPS sessionThis document presents the results from our spectroscopic survey o...
We present the spectroscopic study of 5 Herbig Ae/Be stars in young open clusters. These are identif...
We present the results of a search for Be stars in six fields centered on the young clusters NGC 330...
Proceedings corresponding to poster 581 from the Special Session 7 about young stellar objects at th...
With the Palomar Transient Factory Survey, we report Be stars candidates in the open cluster NGC 663...
AbstractWe recently launched a comprehensive ground based (ESO/VLT/NTT) and space (HST & SST) study ...
Context.By studying young open clusters, the mechanisms important for star formation over several M...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
International audienceContext. Stellar physical properties of star clusters are poorly known and the...
Abstract. Emission-line stars in young open clusters are identified to study their properties, as a ...