Titlebook: Stellar Astrophysics; A Tribute to Helmut K. S. Cheng,K. C. Leung,T. P. Li Conference proceedings 2003 Springer Science+Business Media Dor

ADAGE

无思维能力

Distribution

痛恨

Case B Binary Evolution Compared to Observed Algolsns were done with and without the assumption of conservative mass transfer, giving very different results for the distributions of mass ratios and orbital periods for the obtained Algols. The conservative model fits the observations poorly by producing far too many Algols with low mass ratios and la

全部逛商店

雪上轻舟飞过

Gamma-Ray Pulsars in Gould Belt and Unidentified Gamma-Ray Sources in Medium LatitudesBelt. If the pulsar birth rate in Gould Belt is 3 × 10..., the gamma-ray pulsars in this region, which can be detected by EGRET, will must be dominated by those pulsars with large inclination angles. We predict that these gamma-ray pulsars should have a wider period P~ (0.5–0.8)s and with a typical age of several million years old.

招惹

Beaming Effects in Gamma-Ray Burstsivistic phase, which typically occurs at time 10 to 30 days. The break is affected by many parameters, especially by the electron energy fraction (&), and the magnetic energy fraction (math). Implication of orphan afterglow surveys on GRB beaming is investigated. The possible existence of a kind of cylindrical jets is also discussed.

亲爱

Antecedent

Properties of Cloudy Bag Strange Starsfining bag is introduced such that Chiral symmetry is conserved. The temperature evolution can provide a possible way to distinguish a compact object between a neutron star, MIT strange star and Cloudy Bag strange star in observations.

Herd-Immunity