Results 61 to 70 of about 539 (174)
Seismic detection of core magnetic fields in red giants using the gravity offset
Astronomy & AstrophysicsContext. Magnetic fields are known to efficiently redistribute angular momentum in stars. Recently, magnetic fields have been measured in the cores of red giant stars using asteroseismology, and it was shown that core magnetic fields, if unaccounted for,
Villate M., Deheuvels S., Ballot J.
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Bolometric corrections of stellar oscillation mode amplitudes as observed by the PLATO mission
Astronomy & AstrophysicsAims. We derive bolometric correction functions for oscillation mode amplitudes observed by the different cameras of the ESA PLATO mission. Such corrections between bolometric (full light) and mission instrument-specific amplitudes enable comparisons to ...
Lund Mikkel N. +2 more
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Asymptotic power spectra and visibilities of damped mixed modes
Astronomy & AstrophysicsRecent observational studies of red giant stars have estimated the visibility of their mixed oscillation modes, which is a proxy of the average energy of these modes.
Müller Jonas +4 more
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Asteroseismology of pulsating DA white dwarfs with fully evolutionary models
EPJ Web of Conferences, 2013 We present a new approach for asteroseismology of DA white dwarfs that consists in the employment of a large set of non-static, physically sound, fully evolutionary models representative of these stars.
Althaus L.G. +3 more
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Astronomy & AstrophysicsContext. Massive stars play a central role in astrophysics, yet their internal structure remains poorly constrained due to uncertainties regarding their core masses, internal rotation, and chemical mixing.
Neuville P. +9 more
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An Observer's View on the Future of Asteroseismology
Frontiers in Astronomy and Space Sciences, 2019 Scientific research is a continuous process, and the speed of future progress can be estimated by the pace of finding explanations for previous research questions. In this observer's based view of stellar pulsation and asteroseismology, we start with the
Margit Paparó
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Asteroseismology with COROT [PDF]
International Astronomical Union Colloquium, 2004 AbstractThe COROT project has been developed in the framework of the CNES small satellite programme, with European and Brazilian cooperation. It will be launched in 2006. It is dedicated to seismology and detection of telluric planets. It will perform relative broad-band photometry in visible light during very long (150 d) observing runs in the same ...
Gérard Vauclair +4 more
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This is the author accepted manuscript version of: Bowman, D.M. and Bugnet, L. (2025) Asteroseismology. In: Mandel, I. (eds.) Encyclopedia of Astrophysics. Vol. 2, pp. 133-153.UK: Elsevier.
Bowman, Dominic M., Bugnet, Lisa
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Influence of Magnetic Activity on the Determination of Stellar Parameters Through Asteroseismology
Frontiers in Astronomy and Space Sciences, 2019 Magnetic activity changes the gravito-acoustic modes of solar-like stars and in particular their frequencies. There is an angular-degree dependence that is believed to be caused by the non-spherical nature of the magnetic activity in the stellar ...
Fernando Pérez Hernández +8 more
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Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC 6866
Astronomy & AstrophysicsContext. Isochrone fitting is a classical method used to determine the ages of open clusters. However, the derived ages depend strongly on the chosen input physics of the stellar models used to deduce the isochrones.
Wang Haotian +4 more
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