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Fitting formulae for the effects of binary interactions on lick indices and colors of stellar popula
[期刊论文] 作者：Zhong-Mu Li,Zhan-Wen Han,
来源：中国天文和天体物理学报：英文版 年份：2009
多于大约 50% 星在二进制代码，而是很星的人口，研究花单身的星星的人口(ssSSP ) 模型，它不考虑二进制相互作用。事实上， ssSSPs 的综合怪癖与有二进制相互作用(bsSSPs ) 的星的人...
[期刊论文] 作者：Bo Wang,Zhan-Wen Han,
来源：天文和天体物理学研究：英文版 年份：2010
Type Ia supernovae(SNe Ia)play an important role in the study of cosmic evolution,especially in cosmology.There are several progenitor models for SNe Ia propose...
A likely candidate of type Ia supernova progenitors： the X-ray pulsating companion of the hot subdwa
[期刊论文] 作者：Bo Wang,Zhan-Wen Han,
来源：天文和天体物理学研究：英文版 年份：2010
HD 49798 is a hydrogen depleted subdwarf O6 star and has an X-ray pulsating companion (RX J0648.0-4418). The X-ray pulsating companion is a massive white dwarf....
[期刊论文] 作者：Shi-Bi PU,Zhan-Wen Han,
来源：天文和天体物理学研究：英文版 年份：2011
We present high quality long slit spectra along the major and minor axes out to 1.5 effective radii of the massive galaxy NGC 4636 taken by the Hobby-Eberly Tel...
[期刊论文] 作者：Xue-Fei Chen,Zhan-Wen Han,
来源：天体物理学报 年份：2004
We have studied the influence of different choices of core-envelope transition point on the final merger of contact binaries with two main-sequence components....
A likely candidate of type Ia supernova progenitors: the X-ray pulsating companion of the hot subdwa
[期刊论文] 作者：Bo Wang,Zhan-Wen Han,
来源：天文和天体物理学研究 年份：2004
HD49798 is a hydrogen depleted subdwarf 06 star and has an X-ray pulsating companion(RX J0648.0-4418).The X-ray pulsating companion is a massive white dwarf.Emp...
[期刊论文] 作者：Zhan-Wen Han,Hong-Wei Ge,Xue-Fei Chen,Hai-Liang Chen,
来源：天文和天体物理学研究 年份：2020
Binary interactions lead to the formation of intriguing objects, such as compact binaries, super-novae, gamma ray bursts, X-ray binaries, pulsars, novae, catacl...
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