起草
发表于 2025-3-23 13:32:27
http://reply.papertrans.cn/89/8819/881887/881887_11.png
Chronological
发表于 2025-3-23 16:08:09
Type IIb Supernovaes of interaction with circumstellar matter. Models suggest that SN IIb arise in stars of modestly high mass, about 10–18 solar masses, probably in binary systems, and that the masses of the collapsing cores are several solar masses.
运动的我
发表于 2025-3-23 19:17:53
http://reply.papertrans.cn/89/8819/881887/881887_13.png
伤心
发表于 2025-3-24 00:17:41
http://reply.papertrans.cn/89/8819/881887/881887_14.png
ICLE
发表于 2025-3-24 03:11:19
0941-7834such data, and an overview of the evolution of stars that brings them to an explosive endpoint. Part 2 goes into more detail on core-collapse and superluminous events: which kinds of stars produce them, and ho978-3-662-57223-8978-3-662-55054-0Series ISSN 0941-7834 Series E-ISSN 2196-9698
stress-test
发表于 2025-3-24 07:20:09
ompressibility of the fluid, essentially requiring that the “scale-height” of the system be much larger than the vertical extent of the fluid. This is a very good approximation in the ocean but obviously much weaker in the atmosphere, where in fact we should, finally, consider the effects of compres
Minikin
发表于 2025-3-24 10:52:19
http://reply.papertrans.cn/89/8819/881887/881887_17.png
独特性
发表于 2025-3-24 16:37:42
http://reply.papertrans.cn/89/8819/881887/881887_18.png
MIME
发表于 2025-3-24 21:21:46
http://reply.papertrans.cn/89/8819/881887/881887_19.png
抓住他投降
发表于 2025-3-25 00:19:24
David Branch,J. Craig Wheelers of deformation, though finite, must be kept small. Topographic effects continue to dominate in this limit if the flow contacts the bottom, but topography is irrelevant if the coastal flow takes place in a surface layer, insulated from the bottom by an inactive deeper layer. Sidewall curvature then