Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Qiu-Yi Luo"'
Autor:
Kousuke Ishihara, Patricio Sanhueza, Fumitaka Nakamura, Masao Saito, Huei-Ru Vivien Chen, Shanghuo Li, Fernando Olguin, Kotomi Taniguchi, Kaho Morii, Xing Lu, Qiu-yi Luo, Takeshi Sakai, Qizhou Zhang
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 95 (2024)
Fragmentation contributes to the formation and evolution of stars. Observationally, high-mass stars are known to form multiple-star systems, preferentially in cluster environments. Theoretically, Jeans instability has been suggested to determine char
Externí odkaz:
https://doaj.org/article/130eac6e4c824ce2bb3aa6080314f6f9
Autor:
Qi-Lao Gu, Tie Liu, Pak Shing Li, Zhi-Qiang Shen, Xunchuan Liu, Junhao Liu, Xing Lu, Julien Montillaud, Sihan Jiao, Mika Juvela, Mark G. Rawlings, Qizhou Zhang, Patrick Koch, Isabelle Ristorcelli, Jean-Sébastien Carriere, David Eden, Zhiyuan Ren, Ken’ichi Tatematsu, Naomi Hirano, Qiu-yi Luo, Xiaofeng Mai, Namitha Issac
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 126 (2024)
We observe the magnetic field morphology toward a nearby star-forming filamentary cloud, G202.3+2.5, using James Clerk Maxwell Telescope/POL-2 850 μ m thermal dust polarization observations with an angular resolution of 14.″4 (∼0.053 pc). The av
Externí odkaz:
https://doaj.org/article/c141581ce1024ea491bbf223d5b4a27b
Autor:
Qiu-yi Luo, Tie Liu, Aaron T. Lee, Stella S. R. Offner, James di Francesco, Doug Johnstone, Mika Juvela, Paul F. Goldsmith, Sheng-Li Qin, Xiaofeng Mai, Xun-chuan Liu, Patricio Sanhueza, Feng-Wei Xu, Ken’ichi Tatematsu, Somnath Dutta, Huei-Ru Vivien Chen, Shanghuo Li, Aiyuan Yang, Sheng-Yuan Liu, Chin-Fei Lee, Naomi Hirano, Chang Won Lee, Dipen Sahu, Hsien Shang, Shih-Ying Hsu, Leonardo Bronfman, Woojin Kwon, M. G. Rawlings, David Eden, Xing Lu, Qi-lao Gu, Zhiyuan Ren, D. Ward-Thompson, Zhi-Qiang Shen
Publikováno v:
The Astrophysical Journal Letters, Vol 952, Iss 1, p L2 (2023)
One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations toward a forming quadruple protostell
Externí odkaz:
https://doaj.org/article/cbaf5b0c3b3f4ec180b5a5b7ff455c2c
Autor:
Dipen Sahu, Sheng-Yuan Liu, Doug Johnstone, Tie Liu, Neal J. Evans II, Naomi Hirano, Ken’ichi Tatematsu, James Di Francesco, Chin-Fei Lee, Kee-Tae Kim, Somnath Dutta, Shih-Ying Hsu, Shanghuo Li, Qiu-Yi Luo, Patricio Sanhueza, Hsien Shang, Alessio Traficante, Mika Juvela, Chang Won Lee, David J. Eden, Paul F. Goldsmith, Leonardo Bronfman, Woojin Kwon, Jeong-Eun Lee, Yi-Jehng Kuan, Isabelle Ristorcelli
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 2, p 156 (2023)
Starless cores represent the initial stage of evolution toward (proto)star formation, and a subset of them, known as prestellar cores, with high density (∼ 10 ^6 cm ^−3 or higher) and being centrally concentrated are expected to be embryos of (pr
Externí odkaz:
https://doaj.org/article/150c9253a8ab415ba7c9af8aaa815fc1
Autor:
Jian-Wen Zhou, Tie Liu, Neal J Evans, Guido Garay, Paul F Goldsmith, Gilberto C Gómez, Enrique Vázquez-Semadeni, Hong-Li Liu, Amelia M Stutz, Ke Wang, Mika Juvela, Jinhua He, Di Li, Leonardo Bronfman, Xunchuan Liu, Feng-Wei Xu, Anandmayee Tej, L K Dewangan, Shanghuo Li, Siju Zhang, Chao Zhang, Zhiyuan Ren, Ken’ichi Tatematsu, Pak Shing Li, Chang Won Lee, Tapas Baug, Sheng-Li Qin, Yuefang Wu, Yaping Peng, Yong Zhang, Rong Liu, Qiu-Yi Luo, Jixing Ge, Anindya Saha, Eswaraiah Chakali, Qizhou Zhang, Kee-Tae Kim, Isabelle Ristorcelli, Zhi-Qiang Shen, Jin-Zeng Li
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 514, pp.6038-6052. ⟨10.1093/mnras/stac1735⟩
Monthly Notices of the Royal Astronomical Society, 2022, 514, pp.6038-6052. ⟨10.1093/mnras/stac1735⟩
We investigate the presence of hub-filament systems in a large sample of 146 active proto-clusters, using H$^{13}$CO$^{+}$ J=1-0 molecular line data obtained from the ATOMS survey. We find that filaments are ubiquitous in proto-clusters, and hub-fila
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30db1fd516edff67630b20525c875c1f
https://doi.org/10.1093/mnras/stac1735
https://doi.org/10.1093/mnras/stac1735
Autor:
Hong-Li Liu, Tie Liu, Neal J Evans II, Ke Wang, Guido Garay, Sheng-Li Qin, Shanghuo Li, Amelia Stutz, Paul F Goldsmith, Sheng-Yuan Liu, Anandmayee Tej, Qizhou Zhang, Mika Juvela, Di Li, Jun-Zhi Wang, Leonardo Bronfman, Zhiyuan Ren, Yue-Fang Wu, Kee-Tae Kim, Chang-Won Lee, Ken’ichi Tatematsu, Maria R Cunningham, Xun-Chuan Liu, Jing-Wen Wu, Tomoya Hirota, Jeong-Eun Lee, Pak-Shing Li, Sung-Ju Kang, Diego Mardones, Isabelle Ristorcelli, Yong Zhang, Qiu-Yi Luo, L Viktor Toth, Hee-weon Yi, Hyeong-Sik Yun, Ya-Ping Peng, Juan Li, Feng-Yao Zhu, Zhi-Qiang Shen, Tapas Baug, L K Dewangan, Eswaraiah Chakali, Rong Liu, Feng-Wei Xu, Yu Wang, Chao Zhang, Jinzeng Li, Jianwen Zhou, Mengyao Tang, Qiaowei Xue, Namitha Issac, Archana Soam, Rodrigo H Álvarez-Gutiérrez
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 511:501-505
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c671e757db870850d1788541917cd1de
https://doi.org/10.1093/mnras/stac039
https://doi.org/10.1093/mnras/stac039
Autor:
Hong-Li Liu, Anandmayee Tej, Tie Liu, Patricio Sanhueza, Sheng-Li Qin, Jinhua He, Paul F Goldsmith, Guido Garay, Sirong Pan, Kaho Morii, Shanghuo Li, Amelia Stutz, Ken’ichi Tatematsu, Feng-Wei Xu, Leonardo Bronfman, Anindya Saha, Namitha Issac, Tapas Baug, L Viktor Toth, Lokesh Dewangan, Ke Wang, Jianwen Zhou, Chang Won Lee, Dongting Yang, Anxu Luo, Xianjin Shen, Yong Zhang, Yue-Fang Wu, Zhiyuan Ren, Xun-Chuan Liu, Archana Soam, Siju Zhang, Qiu-Yi Luo
We present a statistical study of a sample of 17 hub-filament-system (HFS) clouds of high-mass star formation using high-angular resolution ($\sim$1-2 arcsecond) ALMA 1.3mm and 3mm continuum data. The sample includes 8 infrared (IR)-dark and 9 IR-bri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::838e486d44e64654253145d76d28285e
http://arxiv.org/abs/2301.03144
http://arxiv.org/abs/2301.03144
Autor:
Ken'ichi Tatematsu, Eswaraiah Chakali, Feng-Wei Xu, Mika Juvela, E. Mannfors, Qiu-Yi Luo, Qizhou Zhang, S. N. Zhang, Sheng-Li Qin, Lokesh K. Dewangan, Ke Wang, L. Viktor Tóth, Junzhi Wang, Tie Liu, Rong Liu, Zhiyuan Ren, Leonardo Bronfman, Paul F. Goldsmith, T. Baug, Jin-Zeng Li, Shanghuo Li, Pak Shing Li, Jianwen Zhou, X.-W. Liu, Xi Chen, Chang Won Lee, Somnath Dutta, Hong-Li Liu, Yong Zhang, Di Li, Anandmayee Tej, Chao Zhang, Archana Soam, Yuefang Wu, Anindya Saha, Amelia M. Stutz, Namitha Issac, Mengyao Tang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 510:5009-5022
We present new 3-mm continuum and molecular lines observations from the ATOMS survey towards the massive protostellar clump, MM1, located in the filamentary infrared dark cloud (IRDC), G034.43+00.24 (G34). The lines observed are the tracers of either
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e0377f77f253098eb3fe4dc1f6c718e
https://doi.org/10.1093/mnras/stab2757
https://doi.org/10.1093/mnras/stab2757
Autor:
Cunguo Wang, Shaolin Xiong, B. S. Liu, B. B. Wu, H. Gao, J. Y. Liao, H. M. Zhang, R. C. Ma, Y. S. Wang, Y. F. Zhang, Xue-Feng Lu, C. Cai, Lian Tao, Shuinai Zhang, Tong Li, G. H. Gao, S. M. Jia, Tao Luo, M. Wu, X. Y. Song, Bo Li, Wenxiong Li, J. Jin, Xin-Fu Zhao, He-Yang Liu, S. Xiao, Lei Sun, Junqiang Zhang, J. L. Qu, Y. H. Tan, C. K. Li, Y. Nang, Peng Zhang, R. J. Yang, H. W. Liu, N. Sai, Yuan-Yuan Du, Y. G. Zheng, X. X. Li, Z. Chang, Y. B. Chen, Qiu-Yi Luo, Tian-Xiang Chen, Z. W. Li, F. J. Lu, Qingcui Bu, L. M. Song, S. J. Zheng, XiangYang Wen, X. H. Ma, Da-Wei Han, Ya Fang Huang, H. S. Zhao, Yuan You, Qi-Bin Yi, D. K. Zhou, P. J. Wang, W. S. Wang, Ge Ou, Yi Zhang, C. Z. Liu, Sisi Yang, J. Y. Nie, Xin Ren, Liang Zhang, Cheng-Cheng Guo, Ming-Yu Ge, L. Chen, Wan-Chang Zhang, Xiong Li, Yu-Dong Gu, X. J. Liu, Libin Wang, X. L. Cao, Q. Q. Yin, Y. P. Chen, Y. Wang, X. H. Liang, Fuqin Zhang, S. N. Zhang, Y. P. Xu, B. Y. Wu, Xuelong Li, J. Guan, L. D. Kong, Wei Cui, W. C. Zhang, Jia Huo, Gang Li, Wenhan Jiang, Bin Meng, Y. J. Yang, G. C. Xiao
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 504:2168-2180
We report on the Insight-HXMT observations of the new black hole X-ray binary MAXI J1820+070 during its 2018 outburst. Detailed spectral analysis via the continuum fitting method shows an evolution of the inferred spin during its high soft sate. More
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f610acf0b8a262f5dc74917458f962b0
https://doi.org/10.1093/mnras/stab945
https://doi.org/10.1093/mnras/stab945
Autor:
Y. J. Jin, Z. Chang, J. Y. Liao, H. M. Zhang, Y. F. Zhang, X. B. Li, Y. G. Li, Chun-sheng Zhang, Wenhan Jiang, Bo Li, Yu-Xuan Zhu, G. H. Gao, J. Jin, M. Wu, Y. Zhang, Xin-Fu Zhao, Zhi Zhang, Y. H. Tan, Y. X. Zhu, R. C. Shang, C. Cai, B. Lu, Fuqin Zhang, J. K. Deng, S. N. Zhang, W. C. Xue, X. X. Li, Y. G. Zheng, J. F. Zhou, Ming-Yu Ge, X. H. Ma, Wenxiong Li, Tian-Xiang Chen, F. J. Lu, Y. S. Wang, D. K. Zhou, Wei Cui, T. Zhang, Aimei Zhang, Lin Lin, Li-Ming Song, B. S. Liu, Lei Sun, C. Z. Liu, S. J. Zheng, Luhua Jiang, Y. P. Xu, B. B. Wu, X. L. Cao, Tao Luo, XiangYang Wen, Xue-Feng Lu, Bin Meng, S. Xiao, Y. B. Chen, Junqiang Zhang, Tong Li, H. W. Liu, N. Sai, Mao-Shun Li, Yunchao Liu, Sisi Yang, Y. J. Yang, S. M. Jia, Yuan You, L. D. Kong, Songbo Zhang, Cunguo Wang, Qi-Bin Yi, Yu-Dong Gu, Q. Q. Yin, Y. P. Chen, Xuelong Li, J. Guan, X. J. Liu, W. Z. Zhang, Yuan-Yuan Du, Gang Chen, X. H. Liang, G. C. Xiao, R. L. Zhuang, GuoQing Liu, Jia Huo, Y. Nang, Gang Li, Shaolin Xiong, Y. J. Zhang, H. Gao, Qiu-Yi Luo, Z. Zhang, Y. L. Tuo, J. W. Yang, Bing Zhang, B. Y. Wu, Lian Tao, X. Y. Song, H. S. Zhao, G. F. Wang, W. S. Wang, Ge Ou, W. C. Zhang, J. Y. Nie, Yi-Qiao Dong, Cheng-Cheng Guo, C. K. Li, H. Xu, Z. W. Li, Da-Wei Han, Z. L. Zhang, M. X. Fu, Yue Zhang, Ya Fang Huang, J. Z. Wang, L. Chen, Wan-Chang Zhang, Weiguang Cui, Qingcui Bu, Min Gao, J. L. Qu
Publikováno v:
Nature Astronomy. 5:378-384
Fast radio bursts (FRBs) are short pulses observed in radio band from cosmological distances. One class of models invoke soft gamma-ray repeaters (SGRs), or magnetars, as the sources of FRBs. Some radio pulses have been observed from some magnetars,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71ce8a76b222eed2a1860c82215edde6
https://doi.org/10.1038/s41550-021-01302-6
https://doi.org/10.1038/s41550-021-01302-6