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: Mass Outflows from Stars and Galactic Nuclei; Proceedings of the S Luciana Bianchi,Roberto Gilmozzi Conference proceedings 1988 Kluwer Acad

[復制鏈接]
查看: 17705|回復: 60
樓主
發(fā)表于 2025-3-21 17:02:56 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Mass Outflows from Stars and Galactic Nuclei
副標題Proceedings of the S
編輯Luciana Bianchi,Roberto Gilmozzi
視頻videohttp://file.papertrans.cn/626/625246/625246.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Mass Outflows from Stars and Galactic Nuclei; Proceedings of the S Luciana Bianchi,Roberto Gilmozzi Conference proceedings 1988 Kluwer Acad
描述The objective of this workshop was to put together observational and theoretical works on outflows from different kinds of astrophysical objects, occurring on different scales and at various evolutionary phases, and to discuss the impact of observations from future space missions. For the stars, we thought to follow throughout the evolution the relevance (rates and dynamical rrodes) of the mass loss phenomenon, e. g. to explain how and when massive stars loose most of their ini tial mass to end up with typical WD masses. The observations of the solar wind were included for being a unique case where the origin and propagation of the outflow can be resolved. We thought that the comparison with similar phenomena occurring in galactic outflows would be fruitful, as demonstrated by recent works on galactic winds and jets. The interest of having this workshop in Torino came because there are groups in this area, at the Astronomical Observatory and at the Institute of Physics of the University, involved in the theoretical and observational studies of outflows from astrophysical objects. The members of the Scientific Organizing Conmi ttee were: V. Castellani, C. Cesarski, P. Conti, A. Ferr
出版日期Conference proceedings 1988
關鍵詞Galaxy; Quasar; magnetosphere; relativistic jet; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-2941-8
isbn_softcover978-94-010-7824-5
isbn_ebook978-94-009-2941-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightKluwer Academic Publishers 1988
The information of publication is updating

書目名稱Mass Outflows from Stars and Galactic Nuclei影響因子(影響力)




書目名稱Mass Outflows from Stars and Galactic Nuclei影響因子(影響力)學科排名




書目名稱Mass Outflows from Stars and Galactic Nuclei網絡公開度




書目名稱Mass Outflows from Stars and Galactic Nuclei網絡公開度學科排名




書目名稱Mass Outflows from Stars and Galactic Nuclei被引頻次




書目名稱Mass Outflows from Stars and Galactic Nuclei被引頻次學科排名




書目名稱Mass Outflows from Stars and Galactic Nuclei年度引用




書目名稱Mass Outflows from Stars and Galactic Nuclei年度引用學科排名




書目名稱Mass Outflows from Stars and Galactic Nuclei讀者反饋




書目名稱Mass Outflows from Stars and Galactic Nuclei讀者反饋學科排名




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限
沙發(fā)
發(fā)表于 2025-3-21 21:49:17 | 只看該作者
Requirements for Theoretical Models of Outflowsd indisputable evidence for mass loss from the α Her system, the topic of mass loss has grown to be a major research area in astrophysics. The review papers presented at this Workshop summarize the current status of this field.
板凳
發(fā)表于 2025-3-22 01:17:32 | 只看該作者
地板
發(fā)表于 2025-3-22 08:08:10 | 只看該作者
5#
發(fā)表于 2025-3-22 09:52:03 | 只看該作者
Masses of Planetary Nebulae and their Central Starsosity)..The central star mass can only be determined at present from its luminosity and evolutionary considerations. The present status is summarized. A range of masses between 0.5 and 1M are found. Some inconsistancies between theory and observations are discussed.
6#
發(fā)表于 2025-3-22 16:36:26 | 只看該作者
Mass Loss and Post-Asymptotic Giant-Branch Evolutionremnant depends very sensitively on the initial condition prevailing during its formation. By this very reason the somewhat approximative calculations of Paczynski (1971) failed to give a satisfactory explanation of the evolution of the central stars (CPN).
7#
發(fā)表于 2025-3-22 19:26:49 | 只看該作者
0067-0057 ects, occurring on different scales and at various evolutionary phases, and to discuss the impact of observations from future space missions. For the stars, we thought to follow throughout the evolution the relevance (rates and dynamical rrodes) of the mass loss phenomenon, e. g. to explain how and
8#
發(fā)表于 2025-3-23 00:10:22 | 只看該作者
9#
發(fā)表于 2025-3-23 02:49:58 | 只看該作者
10#
發(fā)表于 2025-3-23 06:06:28 | 只看該作者
 關于派博傳思  派博傳思旗下網站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網 吾愛論文網 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經驗總結 SCIENCEGARD IMPACTFACTOR 派博系數 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網安備110108008328) GMT+8, 2025-10-11 05:00
Copyright © 2001-2015 派博傳思   京公網安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
镇康县| 波密县| 平昌县| 青浦区| 凤台县| 曲阜市| 乌鲁木齐县| 新蔡县| 榕江县| 忻城县| 大悟县| 容城县| 闻喜县| 永年县| 航空| 大方县| 麟游县| 久治县| 长寿区| 福安市| 城固县| 临安市| 安仁县| 金山区| 南昌县| 荃湾区| 岢岚县| 建瓯市| 嘉善县| 乌拉特前旗| 台湾省| 东阿县| 永清县| 冕宁县| 绍兴市| 开化县| 阳东县| 达尔| 宁远县| 南溪县| 横山县|