Contains fulltext : 236328.pdf (Publisher’s version ) (Open Access
Contains fulltext : 178476.pdf (publisher's version ) (Open Access
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
© 2019. The American Astronomical Society. All rights reserved.. Uncertainties in stellar structure ...
International audienceABSTRACT Since the end of 2018, the Transiting Exoplanet Survey Satellite (TES...
Light curves and periodograms of 160 B stars observed by the TESS space mission and 29 main-sequence...
Contains fulltext : 194970.pdf (preprint version ) (Open Access
Magnetic chemically peculiar (mCP) stars constitute about 10% of upper-main-sequence stars and are c...
International audienceRecently, high-precision optical 2-min cadence light curves obtained with TESS...
About 10 per cent of upper main-sequence stars are characterized by the presence of chemical peculia...
Context. High-quality light curves from space-based missions have opened up a new window on the rota...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Contains fulltext : 168652.pdf (publisher's version ) (Open Access
International audienceContext. The majority of magnetic chemically peculiar (mCP) stars exhibit peri...
Rotation is a key physical process operating in the A stars. We present a method by which rotation p...
Contains fulltext : 178476.pdf (publisher's version ) (Open Access
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
© 2019. The American Astronomical Society. All rights reserved.. Uncertainties in stellar structure ...
International audienceABSTRACT Since the end of 2018, the Transiting Exoplanet Survey Satellite (TES...
Light curves and periodograms of 160 B stars observed by the TESS space mission and 29 main-sequence...
Contains fulltext : 194970.pdf (preprint version ) (Open Access
Magnetic chemically peculiar (mCP) stars constitute about 10% of upper-main-sequence stars and are c...
International audienceRecently, high-precision optical 2-min cadence light curves obtained with TESS...
About 10 per cent of upper main-sequence stars are characterized by the presence of chemical peculia...
Context. High-quality light curves from space-based missions have opened up a new window on the rota...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Contains fulltext : 168652.pdf (publisher's version ) (Open Access
International audienceContext. The majority of magnetic chemically peculiar (mCP) stars exhibit peri...
Rotation is a key physical process operating in the A stars. We present a method by which rotation p...
Contains fulltext : 178476.pdf (publisher's version ) (Open Access
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
© 2019. The American Astronomical Society. All rights reserved.. Uncertainties in stellar structure ...