Results 121 to 130 of about 5,073 (240)
White-Dwarf Asteroseismology With the Kepler Space Telescope
Frontiers in Astronomy and Space Sciences, 2020 In the course of their evolution, white-dwarf stars go through at least one phase of variability in which the global pulsations they undergo allow astronomers to peer into their interiors, making it possible to shed light on their deep inner structure ...
Alejandro H. Córsico +1 more
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Asteroseismology with Small Telescopes [PDF]
Symposium - International Astronomical Union, 1986 Study of the solar interior through analysis of solar oscillations, a field now referred to as helioseismology, has generated interest in the development of asteroseismology, the study of the interior of pulsating stars through the analysis of their oscillations.
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PBjam: Asteroseismology for everyone
, 2021 Asteroseismology is an exceptional tool for measuring fundamental stellar properties. The CoRoT, Kepler and TESS missions have observed thousands of stars that oscillate in a similar way as our Sun. This allows us to place tight constraints on their mass, radius and even age, which are important for understanding stellar structure and evolution ...
Nielsen, M.B +3 more
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Editorial: Challenges of asteroseismology in the era of space missions
Frontiers in Astronomy and Space Sciences, 2022 Javier Pascual-Granado +3 more
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Inivited talk - Theoretical aspects of asteroseismology [PDF]
Communications in Asteroseismology, 2007 For a few decades, a large international community is working at the development of stellar seismology, intending to open a new window on the structure and evolution of stars, with the necessary parallel development of new observational techniques, modeling tools and methods for diagnostics and interpretation.
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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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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 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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The ET mission to search for earth 2.0s. [PDF]
Innovation (Camb), 2022 Ge J +4 more
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