Titlebook: Cataclysmic Variables and Low-Mass X-Ray Binaries; Proceedings of the 7 Donald Q. Lamb,Joseph Patterson Conference proceedings 1985 D. Reid

大包裹

Cytokines

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

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

外表读作

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

disrupt

,-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

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

Stress