无法治愈 发表于 2025-3-23 12:43:10

http://reply.papertrans.cn/19/1889/188862/188862_11.png

Alienated 发表于 2025-3-23 16:13:13

http://reply.papertrans.cn/19/1889/188862/188862_12.png

deface 发表于 2025-3-23 18:18:26

Supernovae and Pulsarstific career. His own contributions to that history include supernova explosions in close binary systems as an origin for runaway OB stars (most pulsars are also high-velocity objects), and studies of expanding stellar associations that have prompted explanations in terms of supernovae. Of the more

misshapen 发表于 2025-3-24 00:15:57

The Identification of Massive Supernova Progenitorsir rate of occurrence and theoretical considerations on stellar evolution (the latter only for type II supernovae). The pre-explosion masses are derived from the lightcurves (types II and V) and from the absolute magnitude before the explosion (only for type V’s). We find mass ranges of 6 to 16 M.,

独白 发表于 2025-3-24 04:26:30

http://reply.papertrans.cn/19/1889/188862/188862_15.png

Conscientious 发表于 2025-3-24 10:35:05

Vereinigung, Zersetzung, Umsetzung,s that of a young cluster containing stars of ages up to that of an average giant molecular cloud, a few 10. years. A few stars in the solar neighborhood may be low-mass, still pre-main-sequence, products of recently dissipated clouds.

nitric-oxide 发表于 2025-3-24 12:41:19

http://reply.papertrans.cn/19/1889/188862/188862_17.png

Presbyopia 发表于 2025-3-24 15:28:32

http://reply.papertrans.cn/19/1889/188862/188862_18.png

骂人有污点 发表于 2025-3-24 22:58:24

http://reply.papertrans.cn/19/1889/188862/188862_19.png

或者发神韵 发表于 2025-3-25 03:13:29

The Nearest Molecular Cloudsand are the small molecular-cloud component of the interstellar medium. The large internal velocity dispersions indicate that the clouds are not gravitationally bound, and that they have ages of ~ 10. yr.
页: 1 [2] 3 4 5 6
查看完整版本: Titlebook: Birth and Evolution of Massive Stars and Stellar Groups; Proceedings of a Sym Wilfried Boland,Hugo Woerden Conference proceedings 1985 D. R