大包裹
发表于 2025-3-28 14:53:07
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Cytokines
发表于 2025-3-28 19:03:20
Hydrodynamic Simulations of a Combined Hydrogen, Helium Thermonuclear Runaway on a 10 Km Neutron Sta1.0M, 10 km neutron star. Our simulation produced an outburst which lasted about 2000 sec and peak effective temperature was 3 kev. The peak luminosity exceeded 2 x 10. L . A shock wave caused a precursor in the light curve which lasted 10. sec.
细颈瓶
发表于 2025-3-29 02:40:08
COS-B X-Ray Observations of Cygnus X-3220 days the total duration of observation of this source by COS-B. Preliminary results from the last observations are presented which show that:.The last point does not allow to confirm the hypothesis of an apsidal motion as the cause of the short-term changes of the 4.8h period.
PRISE
发表于 2025-3-29 04:54:39
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外表读作
发表于 2025-3-29 09:39:57
The So-What? Making Sense of It All,elope” phase. If this is the case, there should exist a class of detached “pre-cataclysmic” binaries: double nuclei of planetary nebulae, and close binaries containing hot subdwarfs or white dwarfs. The secondary stars should be lower-main-sequence objects, and the orbital periods should be short (<
FLORA
发表于 2025-3-29 12:01:37
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disrupt
发表于 2025-3-29 18:59:10
,-Inner Functions and ,-Contractions,ing the techniques developed by Rappaport, Joss, and Webbink (1982). Our new calculations (see Fig. 1) take into account the combined effects of (i) the gradual breakdown of quasi-equilibrium of the .He abundance in the interior of the secondary, and (ii) the progressive mixture of fresh .He into th
剧毒
发表于 2025-3-29 23:10:46
New Findings on Overtraining Syndrome,ay sources (Verbunt and Zwaan 1981). A simplified stellar evolution code, which describes the mass-losing star as an n= 3/2 polytrope, was developed previously to study the evolution of binaries with a secondary of low mass (0.01 < M/M. < 0.4), when the angular momentum losses are due to gravitation
faucet
发表于 2025-3-29 23:56:30
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Stress
发表于 2025-3-30 05:01:09
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