The Host Galaxy of the Hyperactive Repeating FRB 20240114A: Behind a Galaxy Cluster

被引:4
作者
Chen, Xiang-Lei [1 ,2 ]
Tsai, Chao-Wei [1 ,3 ,4 ]
Li, Di [1 ,5 ]
Wang, Pei [1 ,3 ]
Feng, Yi [6 ,7 ]
Zhang, Jun-Shuo [1 ,4 ]
Li, Guo-Dong [1 ,4 ]
Zhang, Yong-Kun [1 ]
Bao, Lu-Lu [4 ]
Liao, Mai [1 ,8 ]
Zhang, Lu-Dan [1 ,4 ]
Zuo, Pei [1 ]
Bao, Dong-Wei [1 ]
Niu, Chen-Hui [9 ]
Luo, Rui [10 ]
Zhu, Wei-Wei [1 ,4 ]
Zou, Hu [1 ]
Xue, Sui-Jian [1 ]
Zhang, Bing [11 ,12 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 650011, Peoples R China
[2] Chinese Acad Sci, Key Lab Radio Astron & Technolgoy, A20 Datun Rd, Beijing 100101, Peoples R China
[3] Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
[4] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[5] Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
[6] Zhejiang Lab, Res Ctr Astron Comp, Hangzhou 311100, Peoples R China
[7] Zhejiang Univ, Inst Astron, Sch Phys, Hangzhou 310027, Peoples R China
[8] Univ Diego Portales, Av Republ 180, Santiago, Region Metropol, Chile
[9] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
[10] Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, Peoples R China
[11] Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV 89154 USA
[12] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
基金
中国国家自然科学基金;
关键词
FAST RADIO-BURST; STAR-FORMATION HISTORIES; ALL-SKY SURVEY; IONIZED-GAS; DUST ATTENUATION; ELECTRON-DENSITY; LINE GALAXIES; DATA RELEASE; MILKY-WAY; ULTRAVIOLET;
D O I
10.3847/2041-8213/adadfd
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the optical spectroscopic observations of the host galaxy of the hyperactive repeating fast radio burst (FRB) FRB 20240114A. The host galaxy is a dwarf galaxy at a redshift of z = 0.1306 +/- 0.0002. With a rest-frame coverage of 4300-7900 & Aring;, we have detected H alpha, H beta, [O iii] lambda lambda 4959,5007, [N ii]lambda lambda 6548,6583, and [S ii] lambda 6716 emission lines. The emission line ratios suggest that the ionization in the host galaxy is dominated by star formation. The star formation rate (SFR) derived from the H alpha emission line is (0.06 +/- 0.01) M circle dot yr-1, and the spectral energy distribution fitting suggests the lower limit of the SFR(UV) is 0.09 M circle dot yr-1. The stellar mass is (4.0 +/- 1.8) x 108 M circle dot, making the specific SFR logsSFR(H alpha)=-9.17 +/- 0.07yr-1 . The line ratios indicate an upper limit of a metallicity of 12 + log10([O/H]) similar to 8.5. As the nearest dwarf host galaxy with a repeating FRB, the activity of FRB 20240114A and the properties of this host galaxy closely resemble those of FRB 20121102A and FRB 20190520B. The H alpha-traced dispersion measure provided by the ionized gas of the host galaxy has a moderate contribution of similar to 200 pc cm-3, assuming a warm ionized gas. We found that the distributions of the stellar mass versus SFR are significantly different between repeating and one-off FRBs, as determined by the MANOVA test with p = 0.0116.
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页数:9
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