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20032019
most citedThe MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

232 citations · 2.2k across the 58 of their papers we have counts for

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Showing 2013Show all

8 papers · 1 filter

astro-ph.SR2013

Combining magnetic and seismic studies to constrain processes in massive stars

C. Neiner, P. Degroote, B. Coste +2

The presence of pulsations influences the local parameters at the surface of massive stars and thus it modifies the Zeeman magnetic signatures. Therefore it makes the characterisat…

astro-ph.SR2013

An observational asteroseismic study of the pulsating B-stars in the open cluster NGC 884

S. Saesen, M. Briquet, C. Aerts +2

Recent progress in the seismic interpretation of field β Cep stars has resulted in improvements of the physical description in the stellar structure and evolution model computation…

astro-ph.SR2013★ 1 cited

Magnetic fields in beta Cep, SPB, and Be stars

M. Schoeller, S. Hubrig, M. Briquet +1

Recent observational and theoretical results emphasize the potential significance of magnetic fields for structure, evolution, and environment of massive stars. Depending on their…

astro-ph.IM2013★ 2 cited

Ensemble Asteroseismology of the Young Open Cluster NGC 2244

Conny Aerts, Konstanze Zwintz, Pablo Marcos-Arenal +13

Our goal is to perform in-depth ensemble asteroseismology of the young open cluster NGC2244 with the 2-wheel Kepler mission. While the nominal Kepler mission already implied a revo…

astro-ph.SR2013★ 100 cited

Atmospheric Parameters of 169 F, G, K and M-type Stars in the Kepler Field

J. Molenda-Zakowicz, S. G. Sousa, A. Frasca +15

The asteroseismic and planetary studies, like all research related to stars, need precise and accurate stellar atmospheric parameters as input. We aim at deriving the effective tem…

astro-ph.SR2013★ 32 cited

Two new SB2 binaries with main sequence B-type pulsators in the Kepler field

P. I. Pápics, A. Tkachenko, C. Aerts +15

Context: OB stars are important in the chemistry and evolution of the Universe, but the sample of targets well understood from an asteroseismological point of view is still too lim…