FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153

Based on a high-sensitivity H i survey using the Five-hundred-meter Aperture Spherical radio Telescope, we identified an isolated H i cloud with a system velocity of  ∼127.0 km s ^−1 , which is associated with an optical galaxy KK153 in space. The H i gas of KK153 shows a typical disk-galaxy structu...

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Main Authors: Jin-Long Xu, Ming Zhu, Nai-Ping Yu, Chuan-Peng Zhang, Xiao-Lan Liu, Mei Ai, Peng Jiang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/adbe7e
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author Jin-Long Xu
Ming Zhu
Nai-Ping Yu
Chuan-Peng Zhang
Xiao-Lan Liu
Mei Ai
Peng Jiang
author_facet Jin-Long Xu
Ming Zhu
Nai-Ping Yu
Chuan-Peng Zhang
Xiao-Lan Liu
Mei Ai
Peng Jiang
author_sort Jin-Long Xu
collection DOAJ
description Based on a high-sensitivity H i survey using the Five-hundred-meter Aperture Spherical radio Telescope, we identified an isolated H i cloud with a system velocity of  ∼127.0 km s ^−1 , which is associated with an optical galaxy KK153 in space. The H i gas of KK153 shows a typical disk-galaxy structure. Using the baryonic Tully–Fisher relation, we obtained that the distance to KK153 is 2.0 ${}_{-0.8}^{+1.7}$ Mpc. Adopting this distance, we derived a stellar mass of 4.1 ${}_{-2.6}^{+10.0}\times 1{0}^{5}$ M _⊙ and a neutral gas fraction of 0.63, implying that KK153 is a gas-rich ultrafaint dwarf galaxy in the Local Group or its outskirts. KK153 shows a cool (∼200 K) and warm (∼7400 K) two-phase neutral medium. The g  −  r color distribution of KK153 suggests that new stars are mostly forming in its inner disk. The dynamical mass of KK153 is 6.9 ${}_{-3.0}^{+5.5}\times 1{0}^{7}$ M _⊙ , which is about 60 times larger than its baryonic matter. Detection of such a low-mass and gas-rich halo poses a challenge to the theory of cosmic reionization.
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series The Astrophysical Journal Letters
spelling doaj-art-7ea8b69de17444b98d606fe1a72061e12025-08-20T02:40:32ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019822L3610.3847/2041-8213/adbe7eFAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153Jin-Long Xu0https://orcid.org/0000-0002-7384-797XMing Zhu1https://orcid.org/0000-0001-6083-956XNai-Ping Yu2Chuan-Peng Zhang3https://orcid.org/0000-0002-4428-3183Xiao-Lan Liu4https://orcid.org/0000-0002-1768-9591Mei Ai5Peng Jiang6https://orcid.org/0000-0002-5387-7952National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; xujl@bao.ac.cn; Guizhou Radio Astronomical Observatory, Guizhou University , Guiyang 550000, People’s Republic of ChinaBased on a high-sensitivity H i survey using the Five-hundred-meter Aperture Spherical radio Telescope, we identified an isolated H i cloud with a system velocity of  ∼127.0 km s ^−1 , which is associated with an optical galaxy KK153 in space. The H i gas of KK153 shows a typical disk-galaxy structure. Using the baryonic Tully–Fisher relation, we obtained that the distance to KK153 is 2.0 ${}_{-0.8}^{+1.7}$ Mpc. Adopting this distance, we derived a stellar mass of 4.1 ${}_{-2.6}^{+10.0}\times 1{0}^{5}$ M _⊙ and a neutral gas fraction of 0.63, implying that KK153 is a gas-rich ultrafaint dwarf galaxy in the Local Group or its outskirts. KK153 shows a cool (∼200 K) and warm (∼7400 K) two-phase neutral medium. The g  −  r color distribution of KK153 suggests that new stars are mostly forming in its inner disk. The dynamical mass of KK153 is 6.9 ${}_{-3.0}^{+5.5}\times 1{0}^{7}$ M _⊙ , which is about 60 times larger than its baryonic matter. Detection of such a low-mass and gas-rich halo poses a challenge to the theory of cosmic reionization.https://doi.org/10.3847/2041-8213/adbe7eDwarf galaxiesGalaxy formationGalaxy evolution
spellingShingle Jin-Long Xu
Ming Zhu
Nai-Ping Yu
Chuan-Peng Zhang
Xiao-Lan Liu
Mei Ai
Peng Jiang
FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
The Astrophysical Journal Letters
Dwarf galaxies
Galaxy formation
Galaxy evolution
title FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
title_full FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
title_fullStr FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
title_full_unstemmed FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
title_short FAST Discovery of a Gas-rich and Ultrafaint Dwarf Galaxy: KK153
title_sort fast discovery of a gas rich and ultrafaint dwarf galaxy kk153
topic Dwarf galaxies
Galaxy formation
Galaxy evolution
url https://doi.org/10.3847/2041-8213/adbe7e
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