找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl

[復(fù)制鏈接]
查看: 53466|回復(fù): 63
樓主
發(fā)表于 2025-3-21 19:57:21 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Effects of Mass Loss on Stellar Evolution
副標(biāo)題IAU Colloquium no. 5
編輯C. Chiosi,R. Stalio
視頻videohttp://file.papertrans.cn/303/302865/302865.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl
描述The IAU Colloquium No. 59, "The effects of mass loss on Stellar Evolution" was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du- ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti- cal developments on the problem of mass loss from early ty- pe st
出版日期Book 1981
關(guān)鍵詞Accretion; Galaxy; star; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-8500-1
isbn_softcover978-94-009-8502-5
isbn_ebook978-94-009-8500-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1981
The information of publication is updating

書目名稱Effects of Mass Loss on Stellar Evolution影響因子(影響力)




書目名稱Effects of Mass Loss on Stellar Evolution影響因子(影響力)學(xué)科排名




書目名稱Effects of Mass Loss on Stellar Evolution網(wǎng)絡(luò)公開度




書目名稱Effects of Mass Loss on Stellar Evolution網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Effects of Mass Loss on Stellar Evolution被引頻次




書目名稱Effects of Mass Loss on Stellar Evolution被引頻次學(xué)科排名




書目名稱Effects of Mass Loss on Stellar Evolution年度引用




書目名稱Effects of Mass Loss on Stellar Evolution年度引用學(xué)科排名




書目名稱Effects of Mass Loss on Stellar Evolution讀者反饋




書目名稱Effects of Mass Loss on Stellar Evolution讀者反饋學(xué)科排名




單選投票, 共有 1 人參與投票
 

0票 0.00%

Perfect with Aesthetics

 

0票 0.00%

Better Implies Difficulty

 

1票 100.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 20:52:50 | 只看該作者
板凳
發(fā)表于 2025-3-22 00:39:53 | 只看該作者
Book 1981related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti- cal developments on the problem of mass loss from early ty- pe st
地板
發(fā)表于 2025-3-22 08:18:08 | 只看該作者
Summary, Conclusions, and Future Work,the WR mass loss may also be important for Of stars (Lamers 1980). A determination of the properties of the WR stellar winds will provide diagnostics which might aid in identifying the mass loss mechanism, and P-Cygni profiles form one important data source for this purpose. With the advent of IUE m
5#
發(fā)表于 2025-3-22 12:38:46 | 只看該作者
6#
發(fā)表于 2025-3-22 15:56:36 | 只看該作者
7#
發(fā)表于 2025-3-22 20:25:06 | 只看該作者
8#
發(fā)表于 2025-3-23 00:08:49 | 只看該作者
9#
發(fā)表于 2025-3-23 03:25:34 | 只看該作者
10#
發(fā)表于 2025-3-23 07:50:55 | 只看該作者
An Introduction to Data Mining,± 100 km s.. Our preliminary evaluation of the associated mass loss rate gives 10. M. yr.. Other planetary nebulae nuclei are studied with low resolution IUE spectra and indications are found of mass loss rates consistent with the above value.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-7 19:17
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
揭阳市| 灌阳县| 如皋市| 调兵山市| 勐海县| 泸西县| 罗定市| 泸水县| 靖宇县| 达孜县| 太保市| 汤阴县| 错那县| 皮山县| 托克托县| 马鞍山市| 内乡县| 邵武市| 潜江市| 临武县| 五莲县| 化州市| 怀化市| 武乡县| 五峰| 八宿县| 休宁县| 阜康市| 新蔡县| 沁水县| 栾川县| 石泉县| 萍乡市| 青铜峡市| 洪雅县| 石家庄市| 杨浦区| 巫溪县| 舟曲县| 镇江市| 三明市|