The Megamaser Cosmology Project. XI. A Geometric Distance to CGCG 074-064
文献类型:期刊论文
作者 | Pesce, D. W.1,2; Braatz, J. A.3; Reid, M. J.1; Condon, J. J.3; Gao, F.3,4; Henkel, C.5,6; Kuo, C. Y.7; Lo, K. Y.3; Zhao, W.8,9 |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 2020-02-20 |
卷号 | 890期号:2页码:15 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ab6bcd |
英文摘要 | As part of the survey component of the Megamaser Cosmology Project, we have discovered a disk megamaser system in the galaxy CGCG 074-064. Using the Green Bank Telescope and the Very Large Array, we have obtained spectral monitoring observations of this maser system at a monthly cadence over the course of two years. We find that the systemic maser features display line-of-sight accelerations of similar to 4.4 km s(-1) yr(-1) that are nearly constant with velocity, while the high-velocity maser features show accelerations that are consistent with zero. We have also used the High-Sensitivity Array to make a high-sensitivity very long baseline interferometric map of the maser system in CGCG 074-064, which reveals that the masers reside in a thin, edge-on disk with a diameter of similar to 1.5 mas (0.6 pc). Fitting a three-dimensional warped disk model to the data, we measure a black hole mass of 2.42(-0.20)(+0.22) x 10(7) M-circle dot and a geometric distance to the system of 87.6(-7.2)(+7.9) Mpc. Assuming a cosmic microwave background-frame recession velocity of 7308 +/- 150 km s(-1), we constrain the Hubble constant to = H-0 = 81.0(-6.9)(+7.4) (stat.) +/- 1.4 (sys.) km s(-1) Mpc(-1). |
WOS关键词 | MOLECULAR DISK ; MASER ; GALAXY ; VARIABILITY ; MOTIONS ; FIELD ; JET |
资助项目 | NSF through the Grote Reber Fellowship Program ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000522100700027 |
出版者 | IOP PUBLISHING LTD |
资助机构 | NSF through the Grote Reber Fellowship Program ; NSF through the Grote Reber Fellowship Program ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; NSF through the Grote Reber Fellowship Program ; NSF through the Grote Reber Fellowship Program ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; NSF through the Grote Reber Fellowship Program ; NSF through the Grote Reber Fellowship Program ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; NSF through the Grote Reber Fellowship Program ; NSF through the Grote Reber Fellowship Program ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - John Templeton Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation ; Black Hole Initiative at Harvard University - Gordon and Betty Moore Foundation |
源URL | [http://ir.bao.ac.cn/handle/114a11/55704] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Pesce, D. W. |
作者单位 | 1.Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA 2.Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA 3.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA 4.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China 5.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany 6.King Abdulaziz Univ, Fac Sci, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia 7.Natl Sun Yat Sen Univ, Dept Phys, 70 Lianhai Rd, Kaohsiung 804, Taiwan 8.Shanghai Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 9.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China |
推荐引用方式 GB/T 7714 | Pesce, D. W.,Braatz, J. A.,Reid, M. J.,et al. The Megamaser Cosmology Project. XI. A Geometric Distance to CGCG 074-064[J]. ASTROPHYSICAL JOURNAL,2020,890(2):15. |
APA | Pesce, D. W..,Braatz, J. A..,Reid, M. J..,Condon, J. J..,Gao, F..,...&Zhao, W..(2020).The Megamaser Cosmology Project. XI. A Geometric Distance to CGCG 074-064.ASTROPHYSICAL JOURNAL,890(2),15. |
MLA | Pesce, D. W.,et al."The Megamaser Cosmology Project. XI. A Geometric Distance to CGCG 074-064".ASTROPHYSICAL JOURNAL 890.2(2020):15. |
入库方式: OAI收割
来源:国家天文台
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