Zobrazeno 1 - 5
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pro vyhledávání: '"Kasc Wg"'
Autor:
Sarbani Basu, V. Silva Aguirre, Daniel Huber, William J. Chaplin, Kasc Wg, Andrea Miglio, Tiago L. Campante, Luca Casagrande, A. M. Serenelli
Publikováno v:
Astronomische Nachrichten. 334:22-25
Asteroseismology has been extremely successful in determining the properties of stars in different evolutionary stages with a remarkable level of precision. However, to fully exploit its potential, robust methods for estimating stellar parameters are
Autor:
Kasc Wg, Katrien Kolenberg
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783642296291
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-precision data of these stars are investigated within the RR Lyrae working group as part of the Kepler Asteroseismic Science Consortium (KASC). I present s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::697f55cd5f54ca12d0c0e35cecbe9ab6
https://doi.org/10.1007/978-3-642-29630-7_22
https://doi.org/10.1007/978-3-642-29630-7_22
Autor:
Kasc Wg, K. Uytterhoeven
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783642296291
The Kepler spacecraft is providing photometric time series with micro-magnitude precision for thousands of variable stars, what opens up opportunities to study the pulsational variability in much more detail than was previously possible from the grou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d55fad6b74846a1fcf57cfcffce28cc
https://doi.org/10.1007/978-3-642-29630-7_43
https://doi.org/10.1007/978-3-642-29630-7_43
Autor:
M. P. Di Mauro, G. Doğan, Alfio Bonanno, William J. Chaplin, Mário J. P. F. G. Monteiro, Christoffer Karoff, Dennis Stello, Travis S. Metcalfe, Michael Thompson, Sarbani Basu, Kasc Wg, Patrick Eggenberger
Publikováno v:
Metcalfe et al., T S & Karoff, C 2010, ' Asteroseismology of solar-type stars with Kepler: II. Stellar modeling ', Astronomische Nachrichten, vol. 331, no. 9-10, pp. 977-980 . https://doi.org/10.1002/asna.201011439
Observations from the Kepler satellite were recently published for three bright G-type stars, which were monitored during the first 33.5d of science operations. One of these stars, KIC 11026764, exhibits a characteristic pattern of oscillation freque
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c4aca202abd7d17e5ccf7d5d043509a
http://arxiv.org/abs/1006.5695
http://arxiv.org/abs/1006.5695
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