找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

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

[复制链接]
查看: 10134|回复: 34
发表于 2025-3-21 20:06:03 | 显示全部楼层 |阅读模式
书目名称Wolf-Rayet Stars: Observations, Physics, Evolution
编辑C. W. H. Loore,A. J. Willis
视频video
丛书名称International Astronomical Union Symposia
图书封面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
关键词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

书目名称Wolf-Rayet Stars: Observations, Physics, Evolution影响因子(影响力)




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution影响因子(影响力)学科排名




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution网络公开度




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution网络公开度学科排名




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution被引频次




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution被引频次学科排名




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution年度引用




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution年度引用学科排名




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution读者反馈




书目名称Wolf-Rayet Stars: Observations, Physics, Evolution读者反馈学科排名




单选投票, 共有 0 人参与投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用户组没有投票权限
发表于 2025-3-21 21:31:08 | 显示全部楼层
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
发表于 2025-3-22 03:54:21 | 显示全部楼层
International Astronomical Union Symposiahttp://image.papertrans.cn/w/image/1030105.jpg
发表于 2025-3-22 06:49:03 | 显示全部楼层
https://doi.org/10.1007/978-94-009-7910-9Anomalie; Galaxy; Population; Variation; galaxies; observatory; photometry; planet; spectroscopy; star; star f
发表于 2025-3-22 10:20:13 | 显示全部楼层
发表于 2025-3-22 13:08:23 | 显示全部楼层
发表于 2025-3-22 18:03:27 | 显示全部楼层
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
发表于 2025-3-23 01:15:40 | 显示全部楼层
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
发表于 2025-3-23 05:05:54 | 显示全部楼层
发表于 2025-3-23 09:14:41 | 显示全部楼层
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
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-3 02:24
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表