中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
ON THE RELATIONSHIP OF UC H II REGIONS AND CLASS II METHANOL MASERS. I. SOURCE CATALOGS

文献类型:期刊论文

作者Hu, B.1,2; Menten, K. M.2; Wu, Y.3; Bartkiewicz, A.4; Rygl, K.5; Reid, M. J.6; Urquhart, J. S.7; Zheng, X.8
刊名ASTROPHYSICAL JOURNAL
出版日期2016-12-10
卷号833期号:1页码:9
ISSN号0004-637X
关键词catalogs ISM: molecules masers stars: formation
DOI10.3847/0004-637X/833/1/18
通讯作者Hu, B.(hubonju@gmail.com)
英文摘要We conducted Very Large Array C-configuration observations to measure positions and luminosities of Galactic Class II 6.7 GHz methanol masers and their associated ultra-compact H II regions. The spectral resolution was 3.90625 kHz and the continuum sensitivity reached 45 mu Jy beam(-1). We mapped 372 methanol masers with peak flux densities of more than 2 Jy selected from the literature. Absolute positions have nominal uncertainties of 0 ''.3. In this first paper on the data analysis, we present three catalogs; the first gives information on the strongest feature of 367 methanol maser sources, and the second provides information on all detected maser spots. The third catalog presents derived data of the 127 radio continuum counterparts associated with maser sources. Our detection rate of radio continuum counterparts toward methanol masers is approximately one-third. Our catalogs list properties including distance, flux density, luminosity, and the distribution in the Galactic plane. We found no significant relationship between luminosities of masers and their associated radio continuum counterparts, however, the detection rate of radio continuum emission toward maser sources increases statistically with the maser luminosities.
WOS关键词MASSIVE STAR-FORMATION ; FORMING REGIONS ; VLBI OBSERVATIONS ; BESSEL SURVEY ; HII-REGIONS ; RMS SURVEY ; MILKY-WAY ; GHZ ; KINEMATICS ; ASTROMETRY
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000390334500003
源URL[http://libir.pmo.ac.cn/handle/332002/23392]  
专题中国科学院紫金山天文台
通讯作者Hu, B.
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
2.Max Planck Inst Radioastron, D-53123 Bonn, Germany
3.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
4.Nicolaus Copernicus Univ, Ctr Astron, Fac Phys Astron & Informat, Grudziadzka 5, PL-87100 Torun, Poland
5.Osservatorio Radio Astron INAF ORA, Via P Gobetti 101, I-40129 Bologna, Italy
6.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
7.Univ Kent, Sch Phys Sci, Ingram Bldg, Canterbury CT2 7NH, Kent, England
8.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210008, Jiangsu, Peoples R China
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Hu, B.,Menten, K. M.,Wu, Y.,et al. ON THE RELATIONSHIP OF UC H II REGIONS AND CLASS II METHANOL MASERS. I. SOURCE CATALOGS[J]. ASTROPHYSICAL JOURNAL,2016,833(1):9.
APA Hu, B..,Menten, K. M..,Wu, Y..,Bartkiewicz, A..,Rygl, K..,...&Zheng, X..(2016).ON THE RELATIONSHIP OF UC H II REGIONS AND CLASS II METHANOL MASERS. I. SOURCE CATALOGS.ASTROPHYSICAL JOURNAL,833(1),9.
MLA Hu, B.,et al."ON THE RELATIONSHIP OF UC H II REGIONS AND CLASS II METHANOL MASERS. I. SOURCE CATALOGS".ASTROPHYSICAL JOURNAL 833.1(2016):9.

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