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Titlebook: Kinematics, Dynamics and Structure of the Milky Way; Proceedings of a Wor W. L. H. Shuter Conference proceedings 1983 D. Reidel Publishing

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发表于 2025-3-21 17:34:36 | 显示全部楼层 |阅读模式
书目名称Kinematics, Dynamics and Structure of the Milky Way
副标题Proceedings of a Wor
编辑W. L. H. Shuter
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Kinematics, Dynamics and Structure of the Milky Way; Proceedings of a Wor W. L. H. Shuter Conference proceedings 1983 D. Reidel Publishing
描述The idea of holding this workshop on "The Jllilky Way" arose at the conference dinner of a meeting on "Regions of Recent Star Formation" held at Penticton in June 1981. Leo Blitz (now at the University of Maryland) and I decided that there was a need, and agreed that we would organize one in Vancouver in the Spring of 1982. The purpose of the workshop was to have an intensive exchange of ideas between some of the most active workers in the field regarding the recent work which has been significantly changing our concepts of the Milky Way. To achieve this we limited the number of participants, and planned the program so that there was ample time for discussion. The meeting appeared to work very well, both scientifically and socially, and this volume contains 50 of the 55 papers that were The discussion was very lengthy, but since the papers were presented. written up after the meeting many of the points raised have been in the publications, and it seems pointless to reproduce it incorporated here. Leo and I would like to thank the many people who helped to make the meeting a success: at UBC) and Frank J. Kerr (Provost of MPSE C.V. Finnegan (Dean of Science at the University of Maryl
出版日期Conference proceedings 1983
关键词Galaxy; cosmic ray; galaxies; interstellar matter; milky way; star; star formation; stars; stellar; sun
版次1
doihttps://doi.org/10.1007/978-94-009-7060-1
isbn_softcover978-94-009-7062-5
isbn_ebook978-94-009-7060-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1983
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The Coordination of Space and Ground-Based Parallax Programs for Improvement of the Stellar Luminoss a maximum at an absolute magnitude of about +6 or nearly one solar mass, and a minimum at slightly fainter values, near one-half solar mass. It has been customary for investigators to adopt the smoothed function of Luyten which increases steadily throughout this range of absolute magnitude. Howeve
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On the Determination of ,,,d the optical observations sample different parts of the Galaxy. The most reliable method for determining .. seems still to be the direct analysis of the radial velocities of stars with known heliocentric distances. The value so found, R. = 10.4.0.7 kpc, is not sensitive to the form of the velocity
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The Velocity Fields of Gas and Stars within Five KPC of the Sun, probable value of the line of sight velocity, Vr, of an element at galactic longitude ℓ and distance projected onto the plane of the galactic disk r = d • cos(b), where d is the distance to the object, can be represented as;.where the coefficients are determined by a least squares fit.
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A Comparison of the Velocity Fields of Young Stellar Objects and of Sharpless H II Regions,sible to represent the radial component of the smooth field by a formula with a small number of parameters, which can be derived from the observations by standard statistical methods. This has been performed for 1) a list of 989 O- and B-type stars in the solar neighbourhood for which the distance a
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