Search Results - "Lebre, Agnès"
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Surface magnetism in the pulsating RV Tauri star R Scuti
Published in Monthly notices of the Royal Astronomical Society (02-05-2023)“…ABSTRACT We present the surface magnetic field conditions of the brightest pulsating RV Tauri star, R Sct. Our investigation is based on the longest…”
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Determining rotational and macroturbulent velocities of cool magnetic giant stars
Published in Astronomische Nachrichten (01-06-2020)“…An original method of estimating the projected rotational velocity, vsini, and the macroturbulent velocity, vmac, of evolved M giant stars is presented. It is…”
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The evolution of surface magnetic fields in young solar-type stars II: the early main sequence (250–650 Myr)
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract There is a large change in surface rotation rates of sun-like stars on the pre-main sequence and early main sequence. Since these stars have…”
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First detection of surface magnetic fields in post-AGB stars: the cases of U Monocerotis and R Scuti
Published in Monthly notices of the Royal Astronomical Society (11-01-2015)“…While several observational investigations have revealed the presence of magnetic fields in the circumstellar envelopes, jets and outflows of post-asymptotic…”
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The evolution of surface magnetic fields in young solar-type stars – I. The first 250 Myr
Published in Monthly notices of the Royal Astronomical Society (21-03-2016)“…The surface rotation rates of young solar-type stars vary rapidly with age from the end of the pre-main sequence through the early main sequence. Important…”
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The origins of the magnetic field in tip-RGB, AGB and post-AGB stars
Published 24-07-2024“…During the last decade and a half, the new generation spectropolarimeter Narval at Pic du Midi, France allowed the study of weak magnetic fields in cool giant…”
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Surface magnetism in the pulsating RV Tauri star R Scuti
Published 13-05-2023“…Monthly Notices of the Royal Astronomical Society, Volume 522, Issue 3, July 2023, Pages 3861-3876 We present the surface magnetic field conditions of the…”
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Science cases for a visible interferometer
Published 07-03-2017“…High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited…”
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Determining rotational and macroturbulent velocities of cool magnetic giant stars
Published 02-02-2022“…Astronomische Nachrichten, 2020, Volume 341, Issue 5, pp. 486-492 An original method of estimating the projected rotational velocity, $vsini$, and the…”
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Measuring surface magnetic fields of red supergiant stars
Published 26-04-2017“…A&A 603, A129 (2017) RSG stars are very massive cool evolved stars. Recently, a weak magnetic field was measured at the surface of $\alpha$ Ori and this is so…”
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Detection of the linearly polarised spectrum of the red supergiant star alpha Ori
Published 07-02-2017“…In the solar limb, linear polarisation is due to anisotropy of the radiation field induced by limb darkening. It is maximal when it is seen parallel to the…”
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Shock-Induced Polarized Hydrogen Emission Lines in the Mira Star omicron Ceti
Published 29-09-2011“…In the spectra of pulsating stars, especially Mira stars, the detection of intense hydrogen emission lines has been explained by a radiative shock wave,…”
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Stellar Physics with High-Resolution UV Spectropolarimetry
Published 05-08-2019“…Current burning issues in stellar physics, for both hot and cool stars, concern their magnetism. In hot stars, stable magnetic fields of fossil origin impact…”
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