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Titlebook: High-Precision Studies of Compact Variable Stars; Steven Bloemen Book 2015 Springer International Publishing Switzerland 2015 Cataclysmic

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發(fā)表于 2025-3-21 16:11:42 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱High-Precision Studies of Compact Variable Stars
編輯Steven Bloemen
視頻videohttp://file.papertrans.cn/427/426696/426696.mp4
概述Nominated for Springer Theses by the Institute of Astronomy, Katholieke Universiteit Leuven.Expanded and partly rewritten version of the original doctoral thesis.Presents measurements of velocities of
叢書名稱Springer Theses
圖書封面Titlebook: High-Precision Studies of Compact Variable Stars;  Steven Bloemen Book 2015 Springer International Publishing Switzerland 2015 Cataclysmic
描述.This book, which is a reworked and updated version of Steven Bloemen’s original PhD thesis, reports on several high-precision studies of compact variable stars. Its strength lies in the large variety of observational, theoretical and instrumentation techniques that are presented and used and paves the way towards new and detailed asteroseismic applications of single and binary subdwarf stars. Close binary stars are studied using high cadence spectroscopic datasets collected with state of the art electron multiplying CCDs and analysed using Doppler tomography visualization techniques. The work touches upon instrumentation, presenting the calibration of a new fast, multi-colour camera installed at the Mercator Telescope on La Palma. The thesis also includes theoretical work on the computation of the temperature range in which stellar oscillations can be driven in subdwarf B-stars. Finally, the highlight of the thesis is the measurement of velocities of stars using only photometric data from NASA‘s Kepler satellite. Doppler beaming causes stars to appear slightly brighter when they move towards us in their orbits, and this subtle effect can be seen in Kepler‘s brightness measurements
出版日期Book 2015
關(guān)鍵詞Cataclysmic Variables; Compact Binary Stars; Compact Variable Stars; DQ Hercules Stars; High-speed Astro
版次1
doihttps://doi.org/10.1007/978-3-319-10283-2
isbn_softcover978-3-319-38404-7
isbn_ebook978-3-319-10283-2Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing Switzerland 2015
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,Mass Ratio from Doppler Beaming and R?mer Delay Versus Ellipsoidal Modulation in the , Data of KOI-ectroscopy covering the orbit of the system, we used 212 days of publicly available . observations and present the first complete light curve fitting to these data, modelling the eclipses and transits, ellipsoidal modulation, reflection, and Doppler beaming. Markov Chain Monte Carlo simulations are
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