中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Detection of 36 GHz Class I Methanol Maser Emission toward NGC 4945

文献类型:期刊论文

作者McCarthy, Tiege P.2,3; Ellingsen, Simon P.2; Chen, Xi4,5; Breen, Shari L.6; Voronkov, Maxim A.3; Qiao, Hai-hua1,4
刊名ASTROPHYSICAL JOURNAL
出版日期2017-09-10
卷号846期号:2
ISSN号0004-637X
关键词Masers Galaxies: Individual (Ngc 4945) Galaxies: Starburst Radio Lines: Ism
DOI10.3847/1538-4357/aa872c
英文摘要We have searched for emission from the 36.2 GHz (4(-1) -> 3(0)E) methanol transition toward NGC 4945, using the Australia Telescope Compact Array. 36.2 GHz methanol emission was detected offset southeast from the Galactic nucleus. The methanol emission is narrow, with a line width <10 km s(-1) and a luminosity five orders of magnitude higher than Galactic class I masers from the same transition. These characteristics combined the with physical separation from the strong central thermal emission suggests that the methanol emission is a maser. This emission is a factor of similar to 90 more luminous than the widespread emission detected from the Milky Way central molecular zone. This is the fourth detection of extragalactic class I emission and the third detection of extragalactic 36.2 GHz maser emission. These extragalactic class I methanol masers do not appear to be simply highly luminous variants of Galactic class I emission and instead appear to trace large-scale regions of low-velocity shocks in molecular gas, which may precede, or be associated with, the early stages of large-scale star formation.
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000410687700004
源URL[http://119.78.226.72/handle/331011/32567]  
专题中国科学院上海天文台
通讯作者McCarthy, Tiege P.
作者单位1.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Shaanxi, Peoples R China
2.Univ Tasmania, Sch Phys Sci, Hobart, Tas 7001, Australia
3.CSIRO, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia
4.GuangZhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
5.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
6.Univ Sydney, Sch Phys, Sydney Inst Astron SIfA, Sydney, NSW 2006, Australia
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McCarthy, Tiege P.,Ellingsen, Simon P.,Chen, Xi,et al. Detection of 36 GHz Class I Methanol Maser Emission toward NGC 4945[J]. ASTROPHYSICAL JOURNAL,2017,846(2).
APA McCarthy, Tiege P.,Ellingsen, Simon P.,Chen, Xi,Breen, Shari L.,Voronkov, Maxim A.,&Qiao, Hai-hua.(2017).Detection of 36 GHz Class I Methanol Maser Emission toward NGC 4945.ASTROPHYSICAL JOURNAL,846(2).
MLA McCarthy, Tiege P.,et al."Detection of 36 GHz Class I Methanol Maser Emission toward NGC 4945".ASTROPHYSICAL JOURNAL 846.2(2017).

入库方式: OAI收割

来源:上海天文台

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