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Titlebook: Wolf-Rayet Stars: Observations, Physics, Evolution; C. W. H. Loore,A. J. Willis Book 1982 International Astronomical Union 1982 Anomalie.G

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發(fā)表于 2025-3-21 20:06:03 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Wolf-Rayet Stars: Observations, Physics, Evolution
編輯C. W. H. Loore,A. J. Willis
視頻videohttp://file.papertrans.cn/1031/1030105/1030105.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Wolf-Rayet Stars: Observations, Physics, Evolution;  C. W. H. Loore,A. J. Willis Book 1982 International Astronomical Union 1982 Anomalie.G
描述The formative ideas for this symposium originated in 1978 at the IAU Symposium No. 83 on "Mass Loss and Evolution of O-type Stars" held at Qualicum Beach, Vancouver Island, Canada - WR stars generally figure prominently in O-star meetings and vice versa! Following general appro- val by the IAU Executive Committee the initial ideas were cemented at a subsequent meeting, IAU Colloquium No. 59 on "The Effects of Mass Loss on Stellar Evolution", held at Miramare, Trieste, Italy in 1980, which was attended by the ma,jority of the present Scientific Organising Committee and at which meeting the outline programme for this symposium was formulated. 1981 was considered an appropriate year in which to hold a meeting on WR stars, since the last IAU Symposium devoted to this stellar class had been held a decade earlier, in Buenos Aires (IAU Sym- posium No. 49), and during this intervening period a wealth of new observational material had been obtained for WR stars together with significant advances on the theoretical front. The venue for this sym- posium was chosen from the requirement, which can be inferred from the above, that a meeting on ‘hot‘ stars take place in an appropriate, sunny clim
出版日期Book 1982
關(guān)鍵詞Anomalie; Galaxy; Population; Variation; galaxies; observatory; photometry; planet; spectroscopy; star; star f
版次1
doihttps://doi.org/10.1007/978-94-009-7910-9
isbn_softcover978-90-277-1470-1
isbn_ebook978-94-009-7910-9Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1982
The information of publication is updating

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Book 1982ach, Vancouver Island, Canada - WR stars generally figure prominently in O-star meetings and vice versa! Following general appro- val by the IAU Executive Committee the initial ideas were cemented at a subsequent meeting, IAU Colloquium No. 59 on "The Effects of Mass Loss on Stellar Evolution", held
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International Astronomical Union Symposiahttp://image.papertrans.cn/w/image/1030105.jpg
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https://doi.org/10.1007/978-94-009-7910-9Anomalie; Galaxy; Population; Variation; galaxies; observatory; photometry; planet; spectroscopy; star; star f
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Book 1982ealth of new observational material had been obtained for WR stars together with significant advances on the theoretical front. The venue for this sym- posium was chosen from the requirement, which can be inferred from the above, that a meeting on ‘hot‘ stars take place in an appropriate, sunny clim
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1743-9213 r this sym- posium was chosen from the requirement, which can be inferred from the above, that a meeting on ‘hot‘ stars take place in an appropriate, sunny clim978-90-277-1470-1978-94-009-7910-9Series ISSN 1743-9213 Series E-ISSN 2352-2186
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The Science and Impacts of Climate Change — Conclusions from the Second IPCC Assessment Reportce, because the strongly differing time-scales of climate system components like atmosphere, ocean, vegetation, land-ice, and distribution of continents provoke changes in mean values and statistics of deviations from these means on all time-scales longer than the slowest component’ s turn around ti
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