ON THE RELATIONSHIP OF UC H II REGIONS AND CLASS II METHANOL MASERS. I. SOURCE CATALOGS | |
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 |
2016-12-10 | |
卷号 | 833期号:1页码:9 |
关键词 | catalogs ISM: molecules masers stars: formation |
ISSN号 | 0004-637X |
DOI | 10.3847/0004-637X/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 |
内容类型 | 期刊论文 |
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 |
推荐引用方式 GB/T 7714 | 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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