不如屎壳郎
发表于 2025-3-25 07:11:05
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储备
发表于 2025-3-25 09:42:53
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EWE
发表于 2025-3-25 14:14:27
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defeatist
发表于 2025-3-25 17:02:55
Conference proceedings 1985e meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi zing a meeting in Massachusetts in the middle
柔美流畅
发表于 2025-3-26 00:01:53
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Ostrich
发表于 2025-3-26 01:21:18
Anny M. S. Cheng,Scheffer C. G. Tsengconfirmed by the detection of a dozen cataclysmic variables by the EINSTEIN X-ray satellite . We show that the ratio of the formation rates of cataclysmic binaries and LMBX’s is appreciably smaller than the ratio of the number of white dwarfs to the number of neutron stars. A more detailed description of our work is given in .
傀儡
发表于 2025-3-26 06:32:34
Evolution of Cataclysmic Binariesused by gravitational radiation and could produce R CrB stars, AM CVn cataclysmic binaries, DB white dwarfs, and Type I Supernovae. Inconsistencies in the standard evolutionary scenario are discussed. It is possible that a binary nature of a star is the necessary condition for a formation of a high surface brightness planetary nebula.
有毛就脱毛
发表于 2025-3-26 08:31:19
Three Body Interactions and Cataclysmic Binaries in Globular Clustersconfirmed by the detection of a dozen cataclysmic variables by the EINSTEIN X-ray satellite . We show that the ratio of the formation rates of cataclysmic binaries and LMBX’s is appreciably smaller than the ratio of the number of white dwarfs to the number of neutron stars. A more detailed description of our work is given in .
Diskectomy
发表于 2025-3-26 12:48:41
A Systematic Study of Magnetic Braking in Low-Mass Binariesal radiation (Rappaport .. 1982). We have extended this code by using a composite polytrope model for the secondary, wherein the structure of the radiative core is described by an n. = 3 polytrope and the convective envelope by an n = 3/2 polytrope. Our results are described in Rappaport .. 1983; this paper is a short summary.
利用
发表于 2025-3-26 20:31:20
Low-Mass X-Ray Binariesof the sun’s disk in Figure 1. This is the smallest known LMXB; the optical companion is slightly larger than the sunspot group and the bow-tie shaped accretion disk is the same size as Saturn’s ring system.