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Titlebook: Evolution of Galaxies Astronomical Observations; Proceedings of the A I. Appenzeller,H. J. Habing,P. Léna Conference proceedings 1989 Sprin

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书目名称Evolution of Galaxies Astronomical Observations
副标题Proceedings of the A
编辑I. Appenzeller,H. J. Habing,P. Léna
视频video
丛书名称Lecture Notes in Physics
图书封面Titlebook: Evolution of Galaxies Astronomical Observations; Proceedings of the A I. Appenzeller,H. J. Habing,P. Léna Conference proceedings 1989 Sprin
描述These eight lectures have been written up in a clear and pedagogical style in order to serve as an introduction for students to fields of modern astrophysical and astronomical research where otherwise textbooks are not available. The first four lectures cover topics in galactic astronomy (formation, structure and evolution of galaxies) and the remaining four are devoted to observational methods and astronomical instrumentation. The lecturers in the European Astrophysical Doctoral Network rank among the most highly respected specialists, and their lectures have been carefully edited and updated before publication.
出版日期Conference proceedings 1989
关键词Galaxy; astronomy; astrophysics; galaxies
版次1
doihttps://doi.org/10.1007/3-540-51315-9
isbn_softcover978-3-662-13741-3
isbn_ebook978-3-540-46194-4Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1989
The information of publication is updating

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Epithelial Abnormalities of the Cervix Uteriroscopy methods. Finally, we will discuss the application of speckle masking to coherent arrays of telescopes. A very interesting example is the 4x8-m ESO VLT, which should yield the fantastic angular resolution of about 2 milli-arcsec.
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0075-8450 dern astrophysical and astronomical research where otherwise textbooks are not available. The first four lectures cover topics in galactic astronomy (formation, structure and evolution of galaxies) and the remaining four are devoted to observational methods and astronomical instrumentation. The lect
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https://doi.org/10.1007/978-3-319-76641-6n be answered by observation if the time is made available for their study by the present and next generation of telescopes. Many key programmes which are now at the very limit of what is possible should become quite straightforward with the new generation of telescopes. Prime among these facilities
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Stellar populations in galaxies: Structure and evolution,
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