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[期刊论文] 作者：Chuan-Peng Zhang,
来源：天文和天体物理学研究：英文版 年份：2013
We investigated the environment of the infrared dust bubble N68 and searched for evidence of triggered star formation in its surroundings.We performed a multiwa...
[期刊论文] 作者：Chuan-Peng Zhang,Jing-Hua Yuan,
来源：天文和天体物理学研究：英文版 年份：2017
Sometimes,early star formation can be found in cold and dense molecular clouds,such as an infrared dark cloud.Considering that star formation often occurs in cl...
[期刊论文] 作者：Chuan-Peng Zhang,Jin-Long Xu,Guang-Xing Li,Li-Gang Hou,Nai-Ping Yu,Peng Jiang,
来源：天文和天体物理学研究:英文版 年份：2021
H Ⅱ regions made of gas ionized by radiations from young massive stars,are widely distributed in the Milky Way.They are tracers for star formation,and their distributions are correlated with the Galactic spiral structure.Radio recombinatio......
[期刊论文] 作者：Nai-Ping Yu,Lei Qian,Chuan-Peng Zhang,Peng Jiang,Jin-Long Xu,Jun-Jie Wang,
来源：天文和天体物理学研究:英文版 年份：2021
We present the first HI 21 cm spectroscopy detection of J030417.78+002827.4,which is an active galactic nucleus(AGN)with an intermediate-mass black hole(IMBH)in...
[会议论文] 作者：Chuan-Peng Zhang,Timea Csengeri,Friedrich Wyrowski,Thushara Pillai,Karl Menten,Jun-Jie Wang,
来源：2015年射电天文前沿与技术研讨会 年份：2015
The fragmentation at the earliest phases is an important process of massive star formation.Investigations of starless cores and prestellar cores are crucial for the origin of stellar initialmass funct...
[会议论文] 作者：Yang Gao,Haitao Xu,Chung K.Law,Di Li,Lei Qian,Zhiyuan Ren,Chuan-Peng Zhang,
来源：分子云与恒星形成2017学术研讨会 年份：2017
Q1:What is turbulence?Why we care about it in star formation?Turbulence:disordered,mixing,vorticular motion of fluids...
[会议论文] 作者：Chung K.Law,Yang Gao,Haitao Xu,Di Li,Lei Qian,Zhiyuan Ren,Chuan-Peng Zhang,
来源：分子云与恒星形成2017学术研讨会 年份：2017
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