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Formation of the Dark Matter–Deficient S0 Galaxy NGC 4111 under the Tidal Interactions

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成果类型:
期刊论文
作者:
Ai, Mei;Zhu, Ming*;Yu, Nai-ping;Xu, Jin-long;Liu, Xiao-lan;...
通讯作者:
Zhu, Ming;Xu, JL
作者机构:
[Xu, Jin-long; Ai, Mei; Xu, JL; Zhu, Ming; Wang, Jie; Yu, Nai-ping; Zhang, Chuan-peng; Zhu, M; Liu, Xiao-lan; Jiang, Peng; Jing, Yingjie] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing, Peoples R China.
[Xu, Jin-long; Ai, Mei; Xu, JL; Zhu, Ming; Yu, Nai-ping; Zhang, Chuan-peng; Zhu, M; Liu, Xiao-lan; Jiang, Peng] Guizhou Univ, Guizhou Radio Astron Observ, Guiyang 550000, Peoples R China.
[Jiao, Qian] Wuhan Polytech Univ, Sch Elect & Elect Engn, Wuhan 430023, Peoples R China.
[Liu, Yao] Qiannan Normal Univ Nationalities, Sch Phys & Elect, Longshan Rd, Tuyun 558000, Peoples R China.
[Liu, Yao] Qiannan Key Lab Radio Astron, Duyun 558000, Guizhou, Peoples R China.
通讯机构:
[Zhu, M; Xu, JL ] C
Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing, Peoples R China.
Guizhou Univ, Guizhou Radio Astron Observ, Guiyang 550000, Peoples R China.
语种:
英文
期刊:
ASTROPHYSICAL JOURNAL LETTERS
ISSN:
2041-8205
年:
2025
卷:
982
期:
2
页码:
L52
基金类别:
China National Key Program for Science and Technology Research and Development of China [2022YFA1602901]; National Natural Science Foundation of China [12373001, 12225303, 12421003, 12033004]; Chinese Academy of Sciences Project for Young Scientists in Basic Research [YSBR-063]; Youth Innovation Promotion Association of CAS; Central Government Funds for Local Scientific and Technological Development [XZ202201YD0020C]; Guizhou Provincial Science and Technology Projects (QKHFQ) [[2023] 003, [2024] 001-1]; National Key R&D Program of China [2018YFE0202900, 2017YFA0402600]; Open Project Program of the Key Laboratory of FAST; Chinese Academy of Sciences
机构署名:
本校为其他机构
院系归属:
电气与电子工程学院
摘要:
We present high-sensitivity and large-scale atomic hydrogen (H i) observations toward lenticular (S0) galaxy NGC 4111 using the Five-hundred-meter Aperture Spherical Radio Telescope. The column-density map shows that NGC 4111 and seven other different types of galaxies share a huge H i gas complex. The data also suggest that NGC 4111 is interacting with seven galaxies. Moreover, we identified a rotating gas disk associated with NGC 4111 from the H i complex. Still, the H i disk rotation direction has deviated from its stellar disk by about 34 .degrees 2, indicating that the NGC 4111 galaxy is ...

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