D
Di Li
Researcher at Chinese Academy of Sciences
Publications - 726
Citations - 20998
Di Li is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Molecular cloud & Star formation. The author has an hindex of 57, co-authored 617 publications receiving 15824 citations. Previous affiliations of Di Li include Space Science Institute & Max Planck Society.
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Structural evolution and late Carboniferous magmatism of the Zhongguai arc in the western Junggar Basin, Northwest China: implications for tectonic evolution of the Junggar Ocean
TL;DR: The structural evolution and late Carboniferous magmatism of the Zhongguai arc offers some new constraints on the tectonic evolution of the Junggar Ocean as discussed by the authors.
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Self‐Assemblies of pH‐Activatable PEGylated Multiarm Poly(lactic acid‐co‐glycolic acid)‐Doxorubicin Prodrugs with Improved Long‐Term Antitumor Efficacies
TL;DR: Two pH-activatable star-shaped prodrugs synthesized through the condensation reaction between Y- or dumbbell-shaped poly(ethylene glycol)-poly(lactic acid-co-glycolic acid) (PEG-PLGA) copolymer and acid-sensitive cis-aconityl-doxorubicin suggest that they provide a favorable approach to construct effective polymeric drug delivery systems for malignancy therapy.
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Intensity distribution function and statistical properties of fast radio bursts
TL;DR: In this article, a statistical analysis on fast radio bursts (FRBs) was carried out and the authors derived a useful intensity distribution function for the 16 non-repeating FRBs detected by the Parkes telescope and the Green Bank Telescope, which can be described as dN/dF obs = (4.1 ± 1.3) × 10 3 F obs −1.1± 0.2 sky −1 d −1, where F obs is the observed radio fluence in units of Jy ms.
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The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333.
Yasuo Doi,Tetsuo Hasegawa,Ray S. Furuya,Simon Coudé,Charles L. H. Hull,Doris Arzoumanian,Pierre Bastien,Michael Chun-Yuan Chen,James Di Francesco,Rachel Friesen,Martin Houde,Shu-ichiro Inutsuka,Steve Mairs,Masafumi Matsumura,Takashi Onaka,Sarah Sadavoy,Yoshito Shimajiri,Mehrnoosh Tahani,Kohji Tomisaka,Chakali Eswaraiah,Patrick M. Koch,Kate Pattle,Chang Won Lee,Motohide Tamura,David Berry,Tao-Chung Ching,Jihye Hwang,Woojin Kwon,Archana Soam,Jia-Wei Wang,Shih-Ping Lai,Keping Qiu,Derek Ward-Thompson,Do-Young Byun,Huei-Ru V. Chen,Wen Ping Chen,Zhiwei Chen,Jungyeon Cho,Minho Choi,Yunhee Choi,Antonio Chrysostomou,Eun Jung Chung,Pham Ngoc Diep,Hao-Yuan Duan,Lapo Fanciullo,Jason Fiege,Erica Franzmann,Per Friberg,Gary A. Fuller,Tim Gledhill,Sarah Graves,Jane Greaves,Matthew Joseph Griffin,Qilao Gu,Ilseung Han,Jennifer Hatchell,Saeko S. Hayashi,Thiem Hoang,Tsuyoshi Inoue,Kazunari Iwasaki,Il-Gyo Jeong,Doug Johnstone,Yoshihiro Kanamori,Ji-hyun Kang,Miju Kang,Sung-ju Kang,Akimasa Kataoka,Koji S. Kawabata,Francisca Kemper,Gwanjeong Kim,Jongsoo Kim,Kee-Tae Kim,K. H. Kim,Mi-Ryang Kim,Shinyoung Kim,Jason M. Kirk,Masato I. N. Kobayashi,Vera Könyves,Takayoshi Kusune,Jungmi Kwon,Kevin Lacaille,Chi-Yan Law,Chin-Fei Lee,Hyeseung Lee,Jeong-Eun Lee,Sang-Sung Lee,Yong-Hee Lee,Dalei Li,Di Li,Hua-bai Li,Hong-Li Liu,Junhao Liu,Sheng-Yuan Liu,Tie Liu,Ilse De Looze,A-Ran Lyo,Brenda C. Matthews,Gerald H. Moriarty-Schieven,Tetsuya Nagata,Fumitaka Nakamura,Hiroyuki Nakanishi,Nagayoshi Ohashi,Geumsook Park,Harriet Parsons,Nicolas Peretto,Tae-Soo Pyo,Lei Qian,Ramprasad Rao,Mark G. Rawlings,Brendan Retter,J. S. Richer,Andrew Rigby,Hiro Saito,Giorgio Savini,Anna M. M. Scaife,Masumichi Seta,Hiroko Shinnaga,Ya-Wen Tang,Yusuke Tsukamoto,Serena Viti,Hongchi Wang,Anthony Peter Whitworth,Hsi-Wei Yen,Hyunju Yoo,Jinghua Yuan,Hyeong-Sik Yun,Tetsuya Zenko,Chuan-Peng Zhang,Guoyin Zhang,Yapeng Zhang,Jianjun Zhou,Lei Zhu,Philippe André,C. Darren Dowell,S. P. S. Eyres,Sam Falle,Sven Van Loo,Jean-François Robitaille +137 more
TL;DR: In this article, the magnetic field structure of NGC 1333 in the Perseus molecular cloud complex from the B-Fields In Star-forming Region Observations (BISTRO) survey with the POL-2 instrument is investigated.
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A new method for constraining molecular cloud thickness: a study of taurus, perseus, and ophiuchus
TL;DR: In this paper, the authors studied the dependence of the CVD on the line-of-sight thickness of molecular clouds, a quantity which cannot be measured by direct means, and they showed that the relation between CVD and the projected separation of cores (L-2D) is sensitive to the cloud thickness.