Add to ORKGWe report monoperiodic variablitity for the four B-type stars HD 131120, HD 105382, HD 138769 and HD 55522, which we explain by rotational modulation rather than by pulsation. Consequently these variables are removed from the list of candidate slowly pulsating B stars
We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemi...
We carry out a comparative study between a sample of confirmed and well-studied B-type pulsators and...
Contains fulltext : 32568.pdf (publisher's version ) (Open Access)We have gathered...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of the variable B...
Abstract. We present ground-based multi-colour Geneva photometry and high-resolution spectra of the ...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of four variable ...
We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsa...
Aims. In order to better model massive B-type stars, we need to understand the physical processes ta...
International audienceThe analysis of the light curves of 48 B-type stars observed by Kepler is pres...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of the variable B...
Aims. In order to better model massive B-type stars, we need to understand the physical processes ta...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
peer reviewedNumerous B stars on the main sequence are found to be variable. These stars have a rela...
Massive stars are important building blocks of the Universe, and their stellar structure and evoluti...
We present a study of absorption line-profile variations in early-B type near-main-sequence stars wi...
We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemi...
We carry out a comparative study between a sample of confirmed and well-studied B-type pulsators and...
Contains fulltext : 32568.pdf (publisher's version ) (Open Access)We have gathered...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of the variable B...
Abstract. We present ground-based multi-colour Geneva photometry and high-resolution spectra of the ...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of four variable ...
We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsa...
Aims. In order to better model massive B-type stars, we need to understand the physical processes ta...
International audienceThe analysis of the light curves of 48 B-type stars observed by Kepler is pres...
We present ground-based multi-colour Geneva photometry and high-resolution spectra of the variable B...
Aims. In order to better model massive B-type stars, we need to understand the physical processes ta...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
peer reviewedNumerous B stars on the main sequence are found to be variable. These stars have a rela...
Massive stars are important building blocks of the Universe, and their stellar structure and evoluti...
We present a study of absorption line-profile variations in early-B type near-main-sequence stars wi...
We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemi...
We carry out a comparative study between a sample of confirmed and well-studied B-type pulsators and...
Contains fulltext : 32568.pdf (publisher's version ) (Open Access)We have gathered...