Death of Massive Stars 作者: International Astronomical Union; Kawai, Nobuyuki; Pian, Elena 出版年: 2012-9 页数: 478 定价: $ 141.25 ISBN: 9781107019799 豆瓣评分 目前无人评价 评价: 写笔记 写书评 加入购书单 分享到 推荐 内容简介 ··· Massive stars end their lives in fiery explosions...
Death of Massive Stars (IAU S279): Supernovae and Gamma-Ray Bursts, Proceedings of the International Astronomical Union (IAU S279), edited by P. W. A. Roming, N. Kawai and E. PianNot Availabledoi:10.1080/00107514.2013.800153WangChih-Yueh...
We recently determined the mass of the most massive star known to the date, R136a1 with a mass at birth 320 times the mass of our sun, as well as the mass of several other stars that are more massive than 150 M. Such massive stars (~150-300 M) may end their life as pair-...
Massive stars end their lives in fiery explosions and are manifest as core collapse supernovae (CCSNe) or gamma-ray bursts (GRBs). In rare cases, a highly stripped massive star explodes and exhibits properties of both CCSNe and GRBs. In contrast, there are clear cases in which no bright...
MASSIVE stars undergo violent deaths, forming the type II supernovae believed to result from gravitational collapse of the stellar cores. Such an event may be recognised by the optical outburst which occurs when the thermal and kinetic energy generated by the collapse propagates to the stellar ...
Astronomers have found a missing link between the explosive deaths of massive stars and the formation of black holes and neutron stars.
time, they can be recycled to make something different. For example, every atom in our bodies was once part of something else. Over time, rocks can become living things and living things, following their demise, can become fossilized rocks. What's true for us is also true for the stars....
大质量恒星的死亡_美国宇航, 钱德拉, 10/23/07_(The Death of a Massive Star _NASA, Chandra, 10/23/07_) 资源编号 :42594373 格式:jpg 文件体积 :63k 分辨率 :516 x 516 爱给网提供海量的免费商用图库 (cc协议)资源素材免费下载, 本次作品为jpg 格式的大质量恒星的死亡_美国宇航, 钱德拉, 10/23/07...
really massive stars are rare (seeThe Stars: A Celestial Census). This is similar to the music business where only a few musicians ever become superstars. Furthermore, many stars with an initial mass much greater than 1.4MSunwill be reduced to that level by the time they die. For example...
Therefore, the chances of a GRB occurring within our galaxy are extremely unlikely, the researchers say. It's thought that stars with low metallicity are less likely to lose mass as they burn and are thus more massive and rotate faster when they die. The more massive a star is, the more...