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Titlebook: Double Stars; Wulff D. Heintz Book 1978 D. Reidel Publishing Company, Dordrecht, Holland 1978 Population.star.star formation.sun

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發(fā)表于 2025-3-21 17:42:38 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Double Stars
編輯Wulff D. Heintz
視頻videohttp://file.papertrans.cn/283/282690/282690.mp4
叢書名稱Geophysics and Astrophysics Monographs
圖書封面Titlebook: Double Stars;  Wulff D. Heintz Book 1978 D. Reidel Publishing Company, Dordrecht, Holland 1978 Population.star.star formation.sun
描述Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob- tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: Th
出版日期Book 1978
關(guān)鍵詞Population; star; star formation; sun
版次1
doihttps://doi.org/10.1007/978-94-009-9836-0
isbn_softcover978-90-277-0886-1
isbn_ebook978-94-009-9836-0
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1978
The information of publication is updating

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發(fā)表于 2025-3-21 23:05:51 | 只看該作者
19th-Century Achievements,raced. Most visual binaries have not completed a revolution since discovery, and therefore, have not been reobserved in the same section of the orbit. To the present-day orbit investigator, 150 yr old measurements still have far more interest than a mere historical, and so the yellowed folio pages o
板凳
發(fā)表于 2025-3-22 01:44:51 | 只看該作者
Three Quarters of This Century,blem, first extragalactic studies with the new Mt. Wilson telescope, the laws of stellar interiors, and the impact of relativity theory upon astronomy — these and other early highlights of 20th-century work are so much connected with the present, that the historical outline can be said here to merge
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發(fā)表于 2025-3-22 20:40:49 | 只看該作者
Interferometric Observation, with the ‘maximum’ visibility of the fringes as given by a monochromatic point source, a double star does not differ if the line joining the stars is perpendicular to that joining the interferometer slits. Minimum visibility occurs when the separation . of the pair (in radians) and the component .
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發(fā)表于 2025-3-23 00:10:59 | 只看該作者
Photographic Positions,rtzsprung (1921). Though the mean error of one measured image is of the order of 0"1 in each coordinate, one plate can accomodate many exposures obtainable in a short time, and an internal plate error of only 0"02 to 0"01 can be reached from 25 to 100 images. The actual errors are somewhat larger, o
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發(fā)表于 2025-3-23 02:09:55 | 只看該作者
The Orbital Elements of a Visual Binary,as is obtained from the relative observations. In the two-body problem with the masses . and ., the radius vector r, and the constant of gravitation ., the relative motion is represented by the second-order differential equation .. Its six scalar constants of integration correspond to six elements w
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發(fā)表于 2025-3-23 08:24:37 | 只看該作者
Dtermination of Visual Binary Orbits,stem, yet in practice there is little resemblance between the methods. The motion of the earth is insignificant (or easily allowed for in the spectroscopic and photometric cases) which greatly simplifies the formalism. On the other hand, the measuring errors are much larger, compared with the quanti
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