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: Microquasars; Proceedings of the T A. J. Castro-Tirado,J. Greiner,J. M. Paredes Conference proceedings 2001 Springer Science+Business Media

[复制链接]
查看: 37939|回复: 60
发表于 2025-3-21 17:28:14 | 显示全部楼层 |阅读模式
书目名称Microquasars
副标题Proceedings of the T
编辑A. J. Castro-Tirado,J. Greiner,J. M. Paredes
视频video
图书封面Titlebook: Microquasars; Proceedings of the T A. J. Castro-Tirado,J. Greiner,J. M. Paredes Conference proceedings 2001 Springer Science+Business Media
描述The Third Microquasar Workshop (or the ‘Fifth‘ Workshop on Galactic Relativ­ istic Jet Sources), was held in Granada, Andalucia (Spain) on 11-13 September 2000. The aim of this workshop in Granada, following the previous Microquasar Workshops in Greenbelt (1997) and Paris (1998) and the Workshops on galactic sources with relativistic jets in Jodrell Bank (1996) and Milton Keynes (1998), was to focus on the theoretical and observational aspects of microquasars. The study of microquasars, the sources in our Galaxy displaying powerful re­ lativistic jets, is a rapidly advancing field in astrophysics. The new instrumentation on ground (MERLIN, SCUBA, VLA, VLT) and aboard satellites (ASCA, BSAX, ISO, IXAE and RXTE) has provided important results, and much more is expected to come from Chandra and XMM-Newton. In the further future, powerful instru­ mentation will come online in the sub-mm (ALMA) and gamma-rays (INTEG­ RAL), extending our coverage to important regions for the study of microquasars. Energy transport via relativistic jets is one of the most important physical mechan­ isms taking place in compact objects. Large efforts have been devoted to properly understand the disk-jet co
出版日期Conference proceedings 2001
关键词Accretion; Galaxy; Quasar; astrophysics; relativistic jet; star
版次1
doihttps://doi.org/10.1007/978-94-010-0700-9
isbn_softcover978-94-010-3828-7
isbn_ebook978-94-010-0700-9
copyrightSpringer Science+Business Media New York 2001
The information of publication is updating

书目名称Microquasars影响因子(影响力)




书目名称Microquasars影响因子(影响力)学科排名




书目名称Microquasars网络公开度




书目名称Microquasars网络公开度学科排名




书目名称Microquasars被引频次




书目名称Microquasars被引频次学科排名




书目名称Microquasars年度引用




书目名称Microquasars年度引用学科排名




书目名称Microquasars读者反馈




书目名称Microquasars读者反馈学科排名




单选投票, 共有 1 人参与投票
 

1票 100.00%

Perfect with Aesthetics

 

0票 0.00%

Better Implies Difficulty

 

0票 0.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用户组没有投票权限
发表于 2025-3-21 20:21:04 | 显示全部楼层
https://doi.org/10.1007/978-94-010-0700-9Accretion; Galaxy; Quasar; astrophysics; relativistic jet; star
发表于 2025-3-22 02:12:42 | 显示全部楼层
发表于 2025-3-22 08:06:55 | 显示全部楼层
Observations of GRS 1915+105 from the USA Experiment on ArgosWe present first results from a monitoring campaign of GRS 1915+105 undertaken with the USA X-ray timing experiment on the ARGOS satellite. A variety of behaviour has been observed, ranging from low, steady X-ray emission to rapid quasi-periodic flaring on timescales of approximately 10–120 seconds.
发表于 2025-3-22 11:18:55 | 显示全部楼层
Identification of the Donor in GRS 1915+105We report on medium-resolution H and K band spectroscopy of GRS 1915+ 105 using the 8m VLT at ESO. We clearly identify absorption bandheads from .CO/.CO. Together with other features we classify the donor as a K-M III star.
发表于 2025-3-22 13:36:32 | 显示全部楼层
On the Mass-Donating Star in GRS 1915+105Geometric constraints and the lack of eclipses in GRS 1915+105 are used to place limits on the mass of the companion star. We rule out any companion with .. > 19.4.. for a black hole mass of .. ≃ 30..
发表于 2025-3-22 18:09:48 | 显示全部楼层
发表于 2025-3-23 00:53:56 | 显示全部楼层
XTE J1550–564: A Superluminal Ejection During the September 1998 OutburstIn 1998 September, the X-ray transient XTE J155072–564 underwent a major outburst in soft and hard X-rays, followed by a radio flare. Australian Long Baseline Array images obtained shortly after the peak in the radio flare showed evolving structure. The components observed have an apparent separation velocity of > 2..
发表于 2025-3-23 02:47:02 | 显示全部楼层
Optical Behaviour of XTE J1550–564 and XTE J1859+226 from Outburst to QuiescenceWe present here the optical light curves of the Soft X-ray Transients XTE J1550–564 and XTEJ1859+226 from outburst to quiescence
发表于 2025-3-23 08:00:12 | 显示全部楼层
Minioutbursts in XTE J1859+226Photometry of the X-ray transient XTE J1859+226, obtained during outburst, showed at least 3 minioutbursts. During the second one, the source exhibited a 0.3 mag modulation with QPO flaring activity during the minimum.
 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, 2025-5-20 06:25
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