Journal of Guangxi Normal University(Natural Science Edition) ›› 2012, Vol. 30 ›› Issue (3): 71-76.
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ZHANG Miao-jing, YANG Jian-hui, PAN Jiang-hong
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[1] 张妙静,张栩宁,潘江洪,等.物质吸积的外赋AGB星参数化模型[J].广西师范大学学报:自然科学版,2009,27(1):17-20. [2] 张妙静,韦怀勇,潘江洪.质量损失对贫金属AGB星表面丰度的影响[J].广西师范大学学报:自然科学版,2008,26(3):17-20. [3] ZHANG Miao-jing,QIU Xiu-qiang,PAN Jiang-hong.The influence of anew model of progenitor staron supernova explosion[J].Chinese Astronomy and Astrophysics,2009,33(4):384-392. [4] WOOSLEY S E,HEGER A,WEAVER T A.The evolution and explosion ofmassive stars[J].Reviews of Mordern Physics,2002,74(4):1015-1071. [5] HEGER A,WOOSLEY S E.Nucleosynthesis and evolution of massive metal-free stars[J].The Astrophysical Journal,2010,724(1):341-373. [6] WOOSLEY S E,WEAVER T A.The evolution and explosion of massive stars.Ⅱ.explosive hydrodynamics and nucleosynthesis[J].The Astrophysical JournalSupplement Series,1995,101(11):181-235. [7] CHEVALIER R A.Neutron star accretion in a supernova[J].AstrophysicalJournal,1989,346(1):847-859. [8] ILIADIS C,D'AURIA J M,STARRFIELD S,et al.Proton-induced thermonuclear reaction rates for A=20-40 nuclei[J].The Astrophysical Journal Supplement Series,2001,134(1):151-171. [9] HOFFMAN R D,WOOSLEY S E,WEAVER T A.Nucleosynthesis below A=100in massive stars[J].The Astrophysical Journal,2001,549(2):1085-1092. [10] SPITE M,CAYREL R,PLEZ B,et al.First star Ⅵ-aburdances of C,N,O,Li and mixing in extremely metal-poor giants.galactic evolution of the light elements[J].Astronomy and Astrophysics,2005,430(2):655-668. [11] 张妙静,丘秀强,潘江洪,等.新前身星模型对超新星爆发的影响[J].天文学报,2009,50(2):145. [12] 王贻仁,张锁春,谢佐恒,等.超新星爆发机制和数值模拟[M].郑州:河南科学出版社,2003. |
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