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: Supernovae and Gamma-Ray Bursters; Kurt W. Weiler Book 2003 Springer-Verlag Berlin Heidelberg 2003 Cosmology.gamma-ray bursts.standard can

[复制链接]
楼主: 法官所用
发表于 2025-3-25 04:04:15 | 显示全部楼层
Classification of Supernovaemplications briefly addressed. Differences between the homogeneous thermonuclear type Ia and similarities among the heterogeneous core-collapse type Ib, Ic and II are highlighted. Transforming type IIb, narrow line type IIn, supernovae associated with GRBs and few peculiar objects are also discussed
发表于 2025-3-25 10:44:18 | 显示全部楼层
Optical Spectra of Supernovae For some supernovae the circumstellar matter is also probed by the observed spectra. Some of this information can be inferred directly from the observed line profiles and fluxes but, because of the Doppler broadening and severe line blending, interpretation often involves the use of .. The emphasis
发表于 2025-3-25 14:11:35 | 显示全部楼层
发表于 2025-3-25 17:30:38 | 显示全部楼层
X-Ray Supernovaeers such as the circumstellar matter density, mass-loss rate of the progenitor, and temperature of the outgoing and reverse shocks can be derived as a function of time. Despite intensive search over the last ∼ 25 years, only 15 supernovae have been detected in X-rays. We review the individual X-ray
发表于 2025-3-25 23:38:25 | 显示全部楼层
Ultraviolet Supernovaeof their ultraviolet properties. Special emphasis is placed on the results obtained for SN1987A in more than fifteen years of assiduous monitoring with both . and .. It is shown that ultraviolet data have led to the clarification of a number of crucial issues such as the nature of the progenitor and
发表于 2025-3-26 03:48:17 | 显示全部楼层
发表于 2025-3-26 05:20:53 | 显示全部楼层
发表于 2025-3-26 11:54:43 | 显示全部楼层
发表于 2025-3-26 16:19:32 | 显示全部楼层
SN1998bw and Hypernovaehter than other radio bright type Ib/c supernovae in radio bands. The extremely broad features in the optical spectra indicate high velocities of ejected matter ∼ 3 × 10. km s. which, combined with the breadth of light curves, lead to an estimated kinetic energy of explosion of ∼ 2−5×10. erg under t
发表于 2025-3-26 20:27:54 | 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, 2025-5-23 02:43
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