Results 81 to 90 of about 2,129 (197)
An Observer's View on the Future of Asteroseismology
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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Editorial: Challenges of asteroseismology in the era of space missions
Javier Pascual-Granado +3 more
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The imprint of star formation on stellar pulsations. [PDF]
Steindl T, Zwintz K, Vorobyov E.
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Radial Oscillations of the HESS J1731-347 Compact Object Imposing the Karmarkar Condition
We model the light HESS J1731-347 compact object (of known stellar mass and radius) within Einstein’s General Relativity, imposing the Karmarkar condition in gravity for anisotropic stars. The three free parameters of the analytic solution are determined
Grigoris Panotopoulos
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The ET mission to search for earth 2.0s. [PDF]
Ge J +4 more
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Influence of Magnetic Activity on the Determination of Stellar Parameters Through Asteroseismology
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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The AFOE—A New Instrument for Asteroseismology [PDF]
R. W. Noyes +4 more
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Starting in 2019, the TESS mission will monitor the northern ecliptic pole for 1 year. Data will be collected at 30-minute and 2-minute cadences, and only a limited amount of slots will be reserved for targets requiring a 20- second cadence.
Prins Saskia +2 more
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