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Titlebook: Language of the Stars; A Discourse on the T Zdeněk Kopal Book 1979 D. Reidel Publishing Company, Dordrecht, Holland 1979 Inclined Orbit.cel

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書(shū)目名稱(chēng)Language of the Stars
副標(biāo)題A Discourse on the T
編輯Zdeněk Kopal
視頻videohttp://file.papertrans.cn/582/581097/581097.mp4
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Language of the Stars; A Discourse on the T Zdeněk Kopal Book 1979 D. Reidel Publishing Company, Dordrecht, Holland 1979 Inclined Orbit.cel
描述Eclipsing Variables - What They can Tell Us and What We can do with Them The aim of the present book will be to provide an introduction to the inter- pretation of the observed light changes of eclipsing binary stars and their analysis for the elements of the respective systems. Whenever we study the properties of any celestial body - be it a planet or a star - all information we wish to gain can reach us through two different channels: their gravitational attraction, and their light. Gravitational interaction between our Earth and its celestial neighbours is, however, measurable only at distances of the order of the dimensions of our solar system; and the only means of communication with the realm of the stars are their nimble-footed photons reaching us - with appropriate time-lag - across the intervening gaps of space. As long as a star is single and emits constant light, it does not constitute a very revealing source of information. A spectrometry of its light can disclose, to be sure, the temperature (colour, or ionization) of the star‘s semi-transparent outer layers, their chemical composition, and prevalent pressure (through Stark effect) or magnetic field (Zeeman effect), it
出版日期Book 1979
關(guān)鍵詞Inclined Orbit; celestial bodies; earth; gravitation; gravity; planet; solar system; spectrometry; star; star
版次1
doihttps://doi.org/10.1007/978-94-009-9466-9
isbn_softcover978-90-277-1044-4
isbn_ebook978-94-009-9466-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1979
The information of publication is updating

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IntroductionThe aim of the present book will be to provide an introduction to the interpretation of the observed light changes of eclipsing binary stars and their analysis for the elements of the respective systems.
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Analysis of the Light Changes in the Frequency-Domain: Distorted Stars, consequently, their distortion is sufficiently small — that (within the limits of observational errors) they can be regarded as spheres; and methods expounded in Chapter V applied to the observations as they stand.
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Error Analysisignify that, in fact, . = 0.123 000… or again that its uncertainty may amount to several units of the third decimal place. The answer is, of course, implied in the photometric observations at the basis of our study — in their quality as well as number — but appropriate procedures for extracting it remain still to be described.
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