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: Instabilities in Luminous Early Type Stars; Proceedings of a Wor Henny J. G. L. M. Lamers,Camiel W. H. Loore Conference proceedings 1987 D.

[復(fù)制鏈接]
查看: 25119|回復(fù): 57
樓主
發(fā)表于 2025-3-21 18:30:28 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Instabilities in Luminous Early Type Stars
副標(biāo)題Proceedings of a Wor
編輯Henny J. G. L. M. Lamers,Camiel W. H. Loore
視頻videohttp://file.papertrans.cn/468/467906/467906.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Instabilities in Luminous Early Type Stars; Proceedings of a Wor Henny J. G. L. M. Lamers,Camiel W. H. Loore Conference proceedings 1987 D.
描述On April 28 1986 Cornelis de Jager reached the age of 65 years. On April 30 he officially retired from the University of Utrecht where he has held a Chair for Stellar Astrophysics, later changed into Space Physics, since 1958. Cees de Jager, as he prefers to be called by his friends, has had an active and successful life in science. His interest in astronomy was raised by his father under the clear skies of Celebes (Indonesia). He started a study in physics and astronomy as a student of the late M. Minnaert in Utrecht during World War II. When in 1943 the occupying forces recruited students who did not want to sign the declaration of loyalty for their war-efforts, Cees and three fellow students went into hiding at the Observatory in Utrecht. During this very "quiet" period van de Hulst developed the theory of the 21 em radiation of neutral hydrogen and de Jager started the observations of variable stars in the pitch dark nights of a country at war. The study of Beta Cepheids rapid- ly awoke his interest which was kept throughout the years. In 1958 he organized an international campaign to observe 12 Lac spectroscopically and photometrically, which was a great success.
出版日期Conference proceedings 1987
關(guān)鍵詞Galaxy; Variation; galaxies; star; stars; stellar; turbulence
版次1
doihttps://doi.org/10.1007/978-94-009-3901-1
isbn_softcover978-94-010-8232-7
isbn_ebook978-94-009-3901-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1987
The information of publication is updating

書目名稱Instabilities in Luminous Early Type Stars影響因子(影響力)




書目名稱Instabilities in Luminous Early Type Stars影響因子(影響力)學(xué)科排名




書目名稱Instabilities in Luminous Early Type Stars網(wǎng)絡(luò)公開度




書目名稱Instabilities in Luminous Early Type Stars網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Instabilities in Luminous Early Type Stars被引頻次




書目名稱Instabilities in Luminous Early Type Stars被引頻次學(xué)科排名




書目名稱Instabilities in Luminous Early Type Stars年度引用




書目名稱Instabilities in Luminous Early Type Stars年度引用學(xué)科排名




書目名稱Instabilities in Luminous Early Type Stars讀者反饋




書目名稱Instabilities in Luminous Early Type Stars讀者反饋學(xué)科排名




單選投票, 共有 0 人參與投票
 

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

您所在的用戶組沒有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 20:29:57 | 只看該作者
Giant Outbursts of the Eta Carinae - P Cygni TypeDuring such an event, the mass loss rate can be of the order of 0.1 M? yr. for several years. We do not yet understand this phenomenon, partly because most relevant theoretical work has been devoted instead to more familiar, less dramatic stellar winds.
板凳
發(fā)表于 2025-3-22 02:57:03 | 只看該作者
Radiation Driven Instabilitiescur in the supersonic parts of the winds, where as many as one hundred e-folds of linear growth can occur during a typical outflow time. The nonlinear growth of such instabilities can possibly account for the observed superionization and X-ray emission in these stars. Developments in the linear theory of these instabilities is reviewed.
地板
發(fā)表于 2025-3-22 05:57:48 | 只看該作者
5#
發(fā)表于 2025-3-22 11:37:22 | 只看該作者
Non Radially Pulsating Wolf-Rayet Stars initial mass 100 M. losing mass through stellar wind. The periods range from half an hour to a feu hours. The duration of this instability phase is rather short, of the order of a feu e-folding times, uhich are of a feu thousand years.
6#
發(fā)表于 2025-3-22 14:53:49 | 只看該作者
https://doi.org/10.1007/978-94-009-3901-1Galaxy; Variation; galaxies; star; stars; stellar; turbulence
7#
發(fā)表于 2025-3-22 18:35:12 | 只看該作者
8#
發(fā)表于 2025-3-23 01:07:23 | 只看該作者
9#
發(fā)表于 2025-3-23 03:52:33 | 只看該作者
Two Comments on the β Cephei Variable 12 LacertaeAccording to a popular notion, the dominant pulsation mode in the g Cephei variables is radial. There is, however, at least one exception to this rule. The exception is 12 Lacertae.
10#
發(fā)表于 2025-3-23 06:22:57 | 只看該作者
978-94-010-8232-7D. Reidel Publishing Company, Dordrecht, Holland 1987
 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, 2026-2-6 02:50
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
成安县| 南投县| 尼木县| 八宿县| 黔南| 桦川县| 廉江市| 恩平市| 淮北市| 新野县| 萨迦县| 寿光市| 类乌齐县| 顺义区| 太康县| 响水县| 利川市| 长治县| 武宁县| 平利县| 白山市| 荣成市| 富平县| 长春市| 安仁县| 泸水县| 象山县| 阳原县| 邵武市| 迭部县| 巴林左旗| 德庆县| 瓦房店市| 榕江县| 汾阳市| 乌拉特前旗| 潼关县| 朝阳市| 化州市| 大悟县| 洪江市|