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: Upper Main Sequence Stars with Anomalous Abundances; Proceedings of the 9 C. R. Cowley,M. M. Dworetsky,C. Mégessier Conference proceedings

[复制链接]
查看: 33150|回复: 64
发表于 2025-3-21 18:44:03 | 显示全部楼层 |阅读模式
书目名称Upper Main Sequence Stars with Anomalous Abundances
副标题Proceedings of the 9
编辑C. R. Cowley,M. M. Dworetsky,C. Mégessier
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Upper Main Sequence Stars with Anomalous Abundances; Proceedings of the 9 C. R. Cowley,M. M. Dworetsky,C. Mégessier Conference proceedings
描述This volume contains papers presented at IAU Colloquium No. 90. at the Crimean Astrophysical Observatory in May of 1985. A few additional contributions are included from authors who for various reasons were unable to attend the meeting. Four years have passed since the last major international conference on chemically peculiar stars of the upper main sequence was held in Liege. Belgium in 1981. Previous conferences were held in 1975 (Vienna. Austria) and in 1965 (Greenbelt. Maryland. USA). As the proceedings of this Colloquium show. the recent availability of ultraviolet spectra of large numbers of normal and chemically peculiar A and B stars is having a major impact on the way we study these objects. and has led to many new. exciting and unanticipated results. Simultaneously. the more traditional study of optical spectra has been advanced through the increasing use of very high spectral resolution with high signal-to-noise detectors. The chemically peculiar (CP) stars on the upper main sequence belong in the standard framework within which we understand stellar evolution and the history of matter. Recent work has made it clear that the unusual chemistry and magnetic structure of t
出版日期Conference proceedings 1986
关键词Apsis; LOPES; Variation; astronomy; astrophysics; observatory; photometry; planet; planetoid; star; star forma
版次1
doihttps://doi.org/10.1007/978-94-009-4714-6
isbn_softcover978-94-010-8597-7
isbn_ebook978-94-009-4714-6Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1986
The information of publication is updating

书目名称Upper Main Sequence Stars with Anomalous Abundances影响因子(影响力)




书目名称Upper Main Sequence Stars with Anomalous Abundances影响因子(影响力)学科排名




书目名称Upper Main Sequence Stars with Anomalous Abundances网络公开度




书目名称Upper Main Sequence Stars with Anomalous Abundances网络公开度学科排名




书目名称Upper Main Sequence Stars with Anomalous Abundances被引频次




书目名称Upper Main Sequence Stars with Anomalous Abundances被引频次学科排名




书目名称Upper Main Sequence Stars with Anomalous Abundances年度引用




书目名称Upper Main Sequence Stars with Anomalous Abundances年度引用学科排名




书目名称Upper Main Sequence Stars with Anomalous Abundances读者反馈




书目名称Upper Main Sequence Stars with Anomalous Abundances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 23:56:23 | 显示全部楼层
发表于 2025-3-22 01:10:48 | 显示全部楼层
发表于 2025-3-22 05:42:31 | 显示全部楼层
The Magnetic Field and other Parameters of the Chemically Peculiar Starsson it is natural that different investigators are interested in working out and improving methods of determination of B.. Especially great attention attracts the method based on using the multicolor Geneva photometry [1]. Cramer and Maeder have found a dependence between B. and parameter Z of multi
发表于 2025-3-22 11:04:27 | 显示全部楼层
Does ν Cep Indicate a Non-axisymmetric Dynamo?ws a period of about 5 years. It is unplausible that this magnetic field is a relic since νCep was formed by expansion of a B-star. We claim here that νCep represents a dynamo exciting a magnetic field which in the average strongly deviates from symmetry about the rotation axis.
发表于 2025-3-22 16:58:44 | 显示全部楼层
发表于 2025-3-22 21:06:10 | 显示全部楼层
发表于 2025-3-22 22:14:30 | 显示全部楼层
Missing Levels and Lines of Astrophysical Importance and singly ionized atoms and t o gi ve rough predictions of missing levels and lines. The amount of data that have been published for these elements after the edition of the Multiple Tables are considerable. For detailed information about sources of new data and compilations the reader is referred
发表于 2025-3-23 04:18:07 | 显示全部楼层
Characteristic Absorption Features in the Spectra of Ap-Si Stars Between 1250 and 1850 Åssible. The contribution of the Si II multiplets is calculated in LTE for a typical overabundance x 10. of silicon. It accounts for only a small part of the observed absorption. Common unidentified structures, smaller than the 1400 Å depression are pointed out.
发表于 2025-3-23 08:37:36 | 显示全部楼层
 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, 2025-6-17 05:37
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