Results 81 to 90 of about 2,129 (197)

An Observer's View on the Future of Asteroseismology

open access: yesFrontiers 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
doaj   +1 more source

Editorial: Challenges of asteroseismology in the era of space missions

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Javier Pascual-Granado   +3 more
doaj   +1 more source

The imprint of star formation on stellar pulsations. [PDF]

open access: yesNat Commun, 2022
Steindl T, Zwintz K, Vorobyov E.
europepmc   +1 more source

Radial Oscillations of the HESS J1731-347 Compact Object Imposing the Karmarkar Condition

open access: yesUniverse
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
doaj   +1 more source

The ET mission to search for earth 2.0s. [PDF]

open access: yesInnovation (Camb), 2022
Ge J   +4 more
europepmc   +1 more source

Influence of Magnetic Activity on the Determination of Stellar Parameters Through Asteroseismology

open access: yesFrontiers 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
doaj   +1 more source

The AFOE—A New Instrument for Asteroseismology [PDF]

open access: bronze, 1993
R. W. Noyes   +4 more
openalex   +1 more source

A small survey of UV-bright stars around the northern ecliptic pole: seeking new p-mode sdB variables for the TESS mission

open access: yesOpen Astronomy, 2019
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
doaj   +1 more source

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