Search Results - "Lebre, Agnès"

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  1. 1

    Surface magnetism in the pulsating RV Tauri star R Scuti by Georgiev, Stefan, Lèbre, Agnès, Josselin, Eric, Mathias, Philippe, Konstantinova-Antova, Renada, Sabin, Laurence

    “…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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  2. 2

    Determining rotational and macroturbulent velocities of cool magnetic giant stars by Georgiev, Stefan, Lèbre, Agnès, Josselin, Eric, Konstantinova‐Antova, Renada, Morin, Julien

    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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  3. 3

    The evolution of surface magnetic fields in young solar-type stars II: the early main sequence (250–650 Myr) by Folsom, C P, Bouvier, J, Petit, P, Lèbre, A, Amard, L, Palacios, A, Morin, J, Donati, J-F, Vidotto, A A

    “…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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  4. 4

    First detection of surface magnetic fields in post-AGB stars: the cases of U Monocerotis and R Scuti by Sabin, L., Wade, G. A., Lèbre, A.

    “…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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  5. 5

    The evolution of surface magnetic fields in young solar-type stars – I. The first 250 Myr by Folsom, C. P., Petit, P., Bouvier, J., Lèbre, A., Amard, L., Palacios, A., Morin, J., Donati, J.-F., Jeffers, S. V., Marsden, S. C., Vidotto, A. A.

    “…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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  6. 6

    The origins of the magnetic field in tip-RGB, AGB and post-AGB stars by Konstantinova-Antova, Renada, Georgiev, Stefan, Lèbre, Agnès, Charbonnel, Corinne, Palacios, Ana, Aurière, Michel

    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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  7. 7

    Surface magnetism in the pulsating RV Tauri star R Scuti by Georgiev, Stefan, Lèbre, Agnès, Josselin, Eric, Mathias, Philippe, Konstantinova-Antova, Renada, Sabin, Laurence

    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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  8. 8
  9. 9

    Determining rotational and macroturbulent velocities of cool magnetic giant stars by Georgiev, Stefan, Lèbre, Agnès, Josselin, Eric, Konstantinova-Antova, Renada, Morin, Julien

    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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  10. 10

    Measuring surface magnetic fields of red supergiant stars by Tessore, Benjamin, Lèbre, Agnès, Morin, Julien, Mathias, Philippe, Josselin, Eric, Aurière, Michel

    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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  11. 11

    Detection of the linearly polarised spectrum of the red supergiant star alpha Ori by Tessore, Benjamin, Lòpez-Ariste, Arturo, Mathias, Philippe, Lèbre, Agnès, Morin, Julien, Josselin, Eric

    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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  12. 12

    Shock-Induced Polarized Hydrogen Emission Lines in the Mira Star omicron Ceti by Fabas, Nicolas, Lèbre, Agnès, Gillet, Denis

    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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