activity
19992023
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 12.9k across the 75 of their papers we have counts for

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18 papers · 1 filter

astro-ph2008★ 4 cited

Abundances of massive stars: some recent developments

T. Morel

Thanks to their usefulness in various fields of astrophysics (e.g. mixing processes in stars, chemical evolution of galaxies), the last few years have witnessed a large increase in…

astro-ph2008★ 28 cited

New insights into the nature of the peculiar star theta Carinae

S. Hubrig, M. Briquet, T. Morel +3

We acquired high resolution spectroscopic and low resolution spectropolarimetric observations to achieve the following goals: a) to improve the orbital parameters to allow a more i…

astro-ph2008★ 59 cited

The neon content of nearby B-type stars and its implications for the solar model problem

T. Morel, K. Butler

The recent downward revision of the solar photospheric abundances now leads to severe inconsistencies between the theoretical predictions for the internal structure of the Sun and…

astro-ph2008★ 123 cited

Nitrogen enrichment, boron depletion and magnetic fields in slowly-rotating B-type dwarfs

T. Morel, S. Hubrig, M. Briquet

Evolutionary models for massive stars, accounting for rotational mixing effects, do not predict any core-processed material at the surface of B dwarfs with low rotational velocitie…

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★ 78 cited

Towards an understanding of the Of?p star HD 191612: optical spectroscopy

Ian D. Howarth, Nolan R. Walborn, Danny J. Lennon +17

We present extensive optical spectroscopy of the early-type magnetic star HD 191612 (O6.5f?pe-O8fp). The Balmer and HeI lines show strongly variable emission which is highly reprod…