Search Results - "Gaulme, P."

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    SURFACE ACTIVITY AND OSCILLATION AMPLITUDES OF RED GIANTS IN ECLIPSING BINARIES by Gaulme, P, Jackiewicz, J, APPOURCHAUX, T, Mosser, B

    Published in The Astrophysical journal (10-04-2014)
    “…Among the 19 red-giant stars belonging to eclipsing binary systems that have been identified in Kepler data, 15 display solar-like oscillations. We study…”
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    Journal Article
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    TESTING THE ASTEROSEISMIC SCALING RELATIONS FOR RED GIANTS WITH ECLIPSING BINARIES OBSERVED BY KEPLER by Gaulme, P., McKeever, J., Jackiewicz, J., Rawls, M. L., Corsaro, E., Mosser, B., Southworth, J., Mahadevan, S., Bender, C., Deshpande, R.

    Published in The Astrophysical journal (01-12-2016)
    “…ABSTRACT Given the potential of ensemble asteroseismology for understanding fundamental properties of large numbers of stars, it is critical to determine the…”
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    RED GIANTS IN ECLIPSING BINARY AND MULTIPLE-STAR SYSTEMS: MODELING AND ASTEROSEISMIC ANALYSIS OF 70 CANDIDATES FROM KEPLER DATA by Gaulme, P, McKeever, J, Rawls, M L, Jackiewicz, J, Mosser, B, Guzik, J A

    Published in The Astrophysical journal (10-04-2013)
    “…Red giant stars are proving to be an incredible source of information for testing models of stellar evolution, as asteroseismology has opened up a window into…”
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    Journal Article
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    SURFACE ACTIVITY AND OSCILLATION AMPLITUDES OF RED GIANTS IN ECLIPSING BINARIES by Gaulme, P, Jackiewicz, J, APPOURCHAUX, T, Mosser, B

    Published in The Astrophysical journal (10-04-2014)
    “…Among the 19 red-giant stars belonging to eclipsing binary systems that have been identified in Kepler data, 15 display solar-like oscillations. We study…”
    Get full text
    Journal Article
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    Magnetic activity of red giants: correlation between the amplitude of solar-like oscillations and chromospheric indicators by Gehan, C, Godoy-Rivera, D, Gaulme, P

    Published 13-03-2024
    “…A&A 686, A93 (2024) Previous studies have found that red giants (RGs) in close binary systems undergoing spin-orbit resonance exhibit an enhanced level of…”
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    Coupling of acoustic waves to clouds in the jovian troposphere by Gaulme, Patrick, Mosser, Benoît

    Published in Icarus (New York, N.Y. 1962) (01-01-2005)
    “…Seismology is the best tool for investigating the interior structure of stars and giant planets. This paper deals with a photometric study of jovian global…”
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    Venus wind map at cloud top level with the MTR/THEMIS visible spectrometer, I: Instrumental performance and first results by Gaulme, Patrick, Schmider, François-Xavier, Grec, Catherine, López Ariste, Arturo, Widemann, Thomas, Gelly, Bernard

    Published in Planetary and space science (01-08-2008)
    “…Solar light gets scattered at cloud top level in Venus’ atmosphere, in the visible range, which corresponds to the altitude of 67 km. We present Doppler…”
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    Towards the true number of flaring giant stars in the Kepler field. Are there flaring specialities associated with the giant nature? by Oláh, K, Kővári, Zs, Günther, M. N, Vida, K, Gaulme, P, Seli, B, Pál, A

    Published 09-01-2021
    “…A&A 647, A62 (2021) We aim to give a reliable estimate of the number of flaring giant stars in the Kepler field. By analyzing the flaring activity of these…”
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    KIC 7955301: a hierarchical triple system with eclipse timing variations and an oscillating red giant by Gaulme, P, Borkovits, T, Appourchaux, T, Pavlovski, K, Spada, F, Gehan, C, Ong, J, Miglio, A, Tkachenko, A, Mosser, B, Vrard, M, Benbakoura, M, Chojnowski, S. D, Perkins, J, Hedlund, A, Jackiewicz, J

    Published 11-10-2022
    “…A&A 668, A173 (2022) KIC 7955301 is a hierarchical triple system with eclipse timing and depth variations discovered by the Kepler mission. It is composed of a…”
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    99 oscillating red-giant stars in binary systems with NASA TESS and NASA Kepler identified from the SB9-Catalogue by Beck, P. G, Mathur, S, Hambleton, K, García, R. A, Steinwender, L, Eisner, N. L, Nascimento, J. -D. do, Gaulme, P, Mathis, S

    Published 27-04-2022
    “…A&A 667, A31 (2022) Oscillating red-giant stars in binary systems are an ideal testbed for investigating the structure and evolution of stars in the advanced…”
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