3 citations · 5 across the 10 of their papers we have counts for
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The seismology programme of CoRoT
E. Michel, A. Baglin, M. Auvergne +1
We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRo…
Pulsating B and Be stars in the Magellanic Clouds
P. D. Diago, J. Gutiérrez-Soto, J. Fabregat +2
Stellar pulsations in main-sequence B-type stars are driven by the -mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability str…
Pulsating B and Be stars in the Magellanic Clouds
P. D. Diago, J. Gutiérrez-Soto, J. Fabregat +2
Stellar pulsations in main-sequence B-type stars are driven by the -mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability str…
The WFI Halpha spectroscopic survey
Christophe Martayan, Dietrich Baade, Juan Fabregat
This document presents the results from our spectroscopic survey of Halpha emitters in galactic and SMC open clusters with the ESO Wide Field Imager in its slitless spectroscopic m…
Variability of B and Be stars in the LMC/SMC: binaries and pulsations
Christophe Martayan, Pascual Diago, Juan Gutiérrez-Soto +5
To study the variability of the 523 B and Be stars observed in the Magellanic clouds with the VLT-FLAMES, we cross-matched the stars of our sample with the photometric database MAC…
On the nature of early-type emission line objects in NGC6611
Christophe Martayan, Michele Floquet, Anne-Marie Hubert +4
The number and the nature of emission line stars in the young open cluster NGC6611 is still the object of debates. Due to the presence of a strong and variable nebulosity in the cl…