Results 151 to 160 of about 14,588 (266)
Asteroseismology with the WIRE satellite [PDF]
Communications in Asteroseismology, 2007 I give a summary of results from the WIRE satellite, which has been used to observe bright stars from 1999-2000 and 2003-2006. The WIRE targets are monitored for up to five weeks with a duty cycle of 30-40%. The aim has been to characterize the flux variation of stars across the Hertzsprung-Russell diagram.
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Photometric Observations of Short Period Variable Stars: EH Librae
Jurnal Fisika FluxEH Librae [BD-00 2911; αJ2000 = 14h58m55.92s; δJ2000 = -0°56'53.01'] is a pulsating variable δ Scuti stars which is located in the constellation of Libra and has a period of 0.0884129 days.
Sulthan Julieri Djumari +3 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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The imprint of star formation on stellar pulsations. [PDF]
Nat Commun, 2022 Steindl T, Zwintz K, Vorobyov E.
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Magnetar QPOs and Neutron Star Crust Elasticity
UniverseThe crust region is a tiny fraction of neutron stars, but it has a variety of physical properties and plays an important role in astronomical observations. One of the properties characterizing the crust is elasticity. In this review, with the approach of
Hajime Sotani
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The ET mission to search for earth 2.0s. [PDF]
Innovation (Camb), 2022 Ge J +4 more
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Finger on the pulse of asteroseismology
Astronomy & Geophysics, 2023 AbstractWarrick Ball highlights some recent discoveries in the context of the past, present and future of ...
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Frontiers in Astronomy and Space Sciences, 2019 Over 2,000 stars were observed for 1 month with a high enough cadence in order to look for acoustic modes during the survey phase of the Kepler mission. Solar-like oscillations have been detected in about 540 stars.
Savita Mathur +10 more
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Dynamics of Large-Scale Solar Flows. [PDF]
Space Sci Rev, 2023 Hotta H +4 more
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