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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, +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.