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Li-Paczynski新星的研究进展(I):理论
王善钦; 戴子高; 吴雪峰
2015
Source Publication天文学进展
Issue2Pages:205-232
Abstract致密星并合(中子星-中子星并合与中子星-黑洞并合)后抛射出的富中子(neutron rich)物质是合成r过程元素(r-process elements)的重要场所之一,近17年来的理论研究认为,这些r过程元素衰变产生的能量在热化后将形成光学-近红外(Optical-NIR)辐射,这种光学-近红外暂现现象被称为"Li-Paczynski新星(Li-Paczynski novae)",简称为"LP新星",由于它们的典型峰值亮度约为典型的新星(novae)亮度的1000倍,因此又被称为"千新星(Kilonovae)"。此外,理论与观测都直接或间接地表明致密星并合在一定条件下会形成持续时间较短(T_...
Language中文
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/14941
CollectionPMO中文期刊
Recommended Citation
GB/T 7714
王善钦,戴子高,吴雪峰. Li-Paczynski新星的研究进展(I):理论[J]. 天文学进展,2015(2):205-232.
APA 王善钦,戴子高,&吴雪峰.(2015).Li-Paczynski新星的研究进展(I):理论.天文学进展(2),205-232.
MLA 王善钦,et al."Li-Paczynski新星的研究进展(I):理论".天文学进展 .2(2015):205-232.
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