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

被引:0
作者
Ai, Mei [1 ,2 ]
Zhu, Ming [1 ,2 ]
Yu, Nai-ping [1 ,2 ]
Xu, Jin-long [1 ,2 ]
Liu, Xiao-lan [1 ,2 ]
Jing, Yingjie [1 ]
Jiao, Qian [3 ]
Liu, Yao [4 ,5 ]
Zhang, Chuan-peng [1 ,2 ]
Wang, Jie [1 ]
Jiang, Peng [1 ,2 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing, Peoples R China
[2] Guizhou Univ, Guizhou Radio Astron Observ, Guiyang 550000, Peoples R China
[3] Wuhan Polytech Univ, Sch Elect & Elect Engn, Wuhan 430023, Peoples R China
[4] Qiannan Normal Univ Nationalities, Sch Phys & Elect, Longshan Rd, Tuyun 558000, Peoples R China
[5] Qiannan Key Lab Radio Astron, Duyun 558000, Guizhou, Peoples R China
基金
国家重点研发计划; 中国国家自然科学基金;
关键词
ATLAS(3D) PROJECT; DWARF GALAXIES; STELLAR MASS; CLUSTERS; SPIRALS; ORIGIN; TRANSFORMATION; LUMINOSITY; MORPHOLOGY; EVOLUTION;
D O I
10.3847/2041-8213/adbeee
中图分类号
P1 [天文学];
学科分类号
0704 ;
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 undergoing a transition from a spiral galaxy to an S0 galaxy by the tidal interactions. The obtained dark matter to stellar mass ratio of NGC 4111 is 3.1 +/- 0.7, which is lower than the average value of the local Universe, implying that the interactions may strip its dark matter. Our results suggest that in a galaxy group environment, tidal interactions have a significant effect on galaxy features.
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页数:7
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