Finally, it will be discussed whether type II supernovae can serve as an explanation of isotopic anomalies found in certain meteoritic inclusions.doi:10.1016/0146-6410(86)90018-9Wolfgang HillebrandtElsevier B.V.Progress in Particle & Nuclear Physics...
1. 第二型超新星 天文词汇 T ... Type I supernova 第一型超新星Type II supernova第二型超新星Tarantula Nebula 蜘蛛星云 ... www.for68.com|基于5个网页 2. 第二类超新星 我们刚刚叙述的,是天文学家所谓的「第二类超新星」 (Type II supernova)的由来 ,这些星球是核心一旦几乎变成全是铁原子 … ...
Type II Supernovae as Probes of Cosmology. Poznanski, D,E Baron,S. Blondin, et al. astro2010: The Astronomy and Astrophysics Decadal Survey . 2010Poznanski, D,E Baron,S. Blondin, et al.Type II Supernovae as Probes of Cosmology. astro2010: The Astronomy and Astrophysics Decadal Survey ...
supernovae: generalsupernovae: individual: SN 2009ddsupernovae: individual: SN 2007pksupernovae: individual: SN 2010ajsupernovae: individual: SN 1995adsupernovae: individual: SN 1996WContext. Core-collapse Supernovae (CC-SNe) descend from progenitors more massive than about 8 M⊙. Because ...
3) SNeⅡ II型超新星 例句>> 4) Ia supernova Ia型超新星5) shell-like supernova remnants 壳型超新星遗迹 例句>> 6) stars-supernova-general 恒星-超新星补充资料:超新星 超新星supernova 光度突然增加数亿倍的巨大恒星爆发。超新星是最壮观的一类变星,是恒星所能经历的规模最大的灾难性爆发。
Related to Type IIa supernova:Type II supernova su·per·no·va (so͞o′pər-nō′və) n.pl.su·per·no·vae(-vē)orsu·per·no·vas A rare celestial phenomenon involving the explosion of a star and resulting in an extremely bright, short-lived object that emits vast amounts ...
Type II Supernova 作者: Russell, Jesse; Cohn, Ronald; 页数: 80 ISBN: 9785510681581 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 我来说两句 短评 ··· 热门 还没人写过短评呢 我要写书评 Type II Supernova的书评 ··· ( 全部0 条 ) 论坛 ··· 在这本书的...
网络第二型超新星 网络释义 1. 第二型超新星 第二型超新星(Type II supernovae) 只有太阳的60亿倍亮,变暗的方式较不规则。在第二型超新星的光谱中可以看到氢的谱线, … web.fg.tp.edu.tw|基于6个网页
The supernova 1987A in the Large Magellanic Cloud is unique with regard to its distance, the fact that we know the properties of the progenitor star, and the detection of neutrinos emitted in the event. Moreover, since SN 1987A is classified as type II supernova and because with, maybe,...
II [19]and IMB[20]detectors, the constraintµν<∼10−12µB is obtained.Similar upper bound has been obtained also in a recent paper [18] by considering neutrino helicity,ipping process through photon Landau damping in a dense relativistic plasma in a supernova core. It has also ...