activity
19942008
most citedThe seismology programme of CoRoT

3 citations · 5 across the 10 of their papers we have counts for

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astro-ph20083 cited

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…

astro-ph20082 cited

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…

astro-ph2008

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…

astro-ph2008

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…

astro-ph2008

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…

astro-ph2007

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…