中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
moleculargasdistributionaroundthesupernovaremnantg40505

文献类型:期刊论文

作者Ji Yang2; Jielong Zhang1; Zhiyong Cai2; Dengrong Lu2; Youheng Tan1
刊名chinesejournalofastronomyandastrophysics
出版日期2006
卷号6期号:2页码:210
ISSN号1009-9271
英文摘要The distribution of dense molecular gas around the supernova rem- nant G40.5-0.5 has been investigated by radio spectroscopic observations in the CO (J=1 - 0) transition. The molecular gas is found to extend over the entire region of G40.5-0.5. A molecular shell, with a diameter of ~ 26′, coincides with the ionized gas as revealed by the cm-radio observations. This coincidence, along with the velocity discontinuity following the shell, provides direct evidence for interaction between the ionized gas and the dense molecular gas. No clear evidence for cosmic-ray accelera- tion can be identified from this SNR as previously suggested, due to positional uncertainty in relating the SNR shell defined by CO to the EGRET gamma-ray sources, GRO J1904+06, from the gamma-ray observations.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/31412]  
专题中国科学院紫金山天文台
作者单位1.中国科学院高能物理研究所
2.中国科学院紫金山天文台
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GB/T 7714
Ji Yang,Jielong Zhang,Zhiyong Cai,et al. moleculargasdistributionaroundthesupernovaremnantg40505[J]. chinesejournalofastronomyandastrophysics,2006,6(2):210.
APA Ji Yang,Jielong Zhang,Zhiyong Cai,Dengrong Lu,&Youheng Tan.(2006).moleculargasdistributionaroundthesupernovaremnantg40505.chinesejournalofastronomyandastrophysics,6(2),210.
MLA Ji Yang,et al."moleculargasdistributionaroundthesupernovaremnantg40505".chinesejournalofastronomyandastrophysics 6.2(2006):210.

入库方式: OAI收割

来源:紫金山天文台

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