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107篇 您的检索式:期刊名="Ap J"
    题名 作者 年代 出处 被引量
1Comparing models of rapidly rotating relativistic stars constructed by two numerical methods显示文摘STERGIOULAS N FRIEDMAN J L 1995AP J1995,444,:1
2The dynamical instability of gaseous masses approaching the Schwarzchild limit in general relativity显示文摘CHANDRASEKHAR S 1964AP J1964,140,:1
3Multiple Soliton Solutions, Soliton-type Solutions and Rational Solutions for the (3 + 1)-dimensional Potential-YTSF Equation显示文摘LIU J G ZENG Z F 2014Indian J Pure Ap Mat2014,45,:1
4The supernova associated with GRB 030329显示文摘DADO S DAR A DERUJULA A 2003Ap J2003,594,:1
5Positive solutions for boundary value problems of nonlinear fractional differential equation显示文摘Bai Zhanbin Lti Haishen 2005J Math Anal Ap pl2005,311,:1
6The type Ic hypemova SN 2003dh/GRB 030329显示文摘MAZZALI P A DENG J TOMINAGA N 2003Ap J2003,599,:1
7The diversity of gamma-ray burst afterglows and the surroundings of massive stars 显示文摘CHWVALIER R A LI Z Y FRANSSON C 2004Ap J2004,606,1:1
8Relativistic r- Modes in slowly rotating neutron stars: numerical analysis in the cowling approximation显示文摘YOSHIDA S LEE U 2002AP J2002,567,:1
9On new generalizations of Hilbert's inequality and their applications显示文摘 Debnath L 2000J Math Anal Ap pl2000,245,:1
10Slowly rotating relativistic stars Ⅱ Models for neutron star and supermassive stars 显示文摘HARTLE J B THORNE K S 1968AP J1968,153,:1
11Jet energy and other parameters for the afterglows of GRB 980703, GRB 990123, GRB 990510, and GRB 991216 determined from modeling of multifrequeney data显示文摘PANAITESCU A KUMAR P 2001Ap J2001,554,:1
12Comparison of the pharmacokinetics of moxidectin ( Equest~ ) and iver- mectin(Eqvalan~ )in horses显示文摘PI~REZ R CABEZAS I GARC~A M 1999J Vet Pharmacol Ther- ap1999,22,3:1
13Exercise training attenu ates aging-associated increases in collagen and collagen crosslink ing of the left but not the right ventricle in the rat 显示文摘Thomas DP Cotter TA Li X 2001Eur J Ap plPhysiol2001,85,12:1
14Neutron stars are giant hypemucleis显示文摘GLENDNNING N K 1985Ap J1985,293,:1
15Wind interaction models for gamma-ray burst afterglows: the case for two types of progenitors 显示文摘CHEVALIER R A LI Z Y 2000Ap J2000,536,:1
16Application of the improved Hartle method for the construction of general relativistic rotating neutron star models显示文摘WEBER F GLENDENNING N K 1992Ap J1992,390,:1
17Gamma-ray burst afterglows from realistic fireballs显示文摘DAI Z G HUANG Y F LU T 1999Ap J1999,520,:1
18Mass and moment - of - inertia peaks in general relativity 显示文摘ADAMS R C WARBTON R D H COHEN J M 1975AP J1975,200,:1
19Uniaxiai omega medium as a physically realizable alternative for the perfectly matched layer显示文摘Tretyakov S A 1998J Electromagn Wave Ap plic1998,12,6:1
20Pectra and light curves of gamma-ray burst afterglows显示文摘SARI R PIRAN T NARAYAN R 1998Ap J1998,497,:1
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