activity
19952023
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 20.8k across the 163 of their papers we have counts for

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Showing 2007Show all

10 papers · 1 filter

astro-ph2007★ 92 cited

A spectroscopic study of southern (candidate) gamma Doradus stars. II. Detailed abundance analysis and fundamental parameters

H. Bruntt, P. De Cat, C. Aerts

The gamma Doradus stars are a recent class of variable main sequence F-type stars located on the red edge of the Cepheid instability strip. They pulsate in gravity modes, and this…

astro-ph2007★ 198 cited

Automated supervised classification of variable stars I. Methodology

J. Debosscher, L. M. Sarro, C. Aerts +4

The fast classification of new variable stars is an important step in making them available for further research. Selection of science targets from large databases is much more eff…

astro-ph2007★ 6 cited

Close-up of primary and secondary asteroseismic CoRoT targets and the ground-based follow-up observations

K. Uytterhoeven, E. Poretti, M. Rainer +13

To optimise the science results of the asteroseismic part of the CoRoT satellite mission a complementary simultaneous ground-based observational campaign is organised for selected…

astro-ph2007★ 43 cited

An evolutionary study of the pulsating subdwarf B eclipsing binary PG1336-018 (NY Vir)

H. Hu, G. Nelemans, R. Østensen +3

The formation of subdwarf B (sdB) stars is not well understood within the current framework of stellar single and binary evolution. In this study, we focus on the formation and evo…

astro-ph2007★ 145 cited

An asteroseismic study of the beta Cephei star theta Ophiuchi: constraints on global stellar parameters and core overshooting

M. Briquet, T. Morel, A. Thoul +5

We present a seismic study of the beta Cephei star theta Ophiuchi. Our analysis is based on the observation of one radial mode, one rotationally split l = 1 triplet and three compo…

astro-ph2007★ 32 cited

On the co-existence of chemically peculiar Bp stars, slowly pulsating B stars and constant B stars in the same part of the H-R diagram

M. Briquet, S. Hubrig, P. De Cat +3

Aims. In order to better model massive B-type stars, we need to understand the physical processes taking place in slowly pulsating B (SPB) stars, chemically peculiar Bp stars, and…