112 citations
- Chinese Academy of SciencesCN10 papers
- Yunnan UniversityCN8 papers
- National Astronomical ObservatoriesCN6 papers
- Korea Astronomy and Space Science InstituteKR5 papers
- National Astronomical Observatory of JapanJP5 papers
- Institute of Astronomy and Astrophysics, Academia SinicaTW4 papers
- Kavli Institute for Theoretical SciencesCN4 papers
- Korea University of Science and TechnologyKR4 papers
- Kyung Hee UniversityKR4 papers
- Peking UniversityCN4 papers
- Shanghai Astronomical ObservatoryCN4 papers
- Sun Yat-sen UniversityCN4 papers
12 papers
Multiscale Dynamical Scenario of High-mass Star Formation in an IRDC Filament G34
Sirong Pan, Hong-Li Liu, Sheng-Li Qin
There is growing evidence that high-mass star formation (HMSF) is a multiscale, dynamical process in molecular clouds, where filaments transport gas material between larger and sma…
Morphological evidence for nanoflares heating warm loops in the solar corona
Y. Bi, J. J. Yang, Y. Qin +6
Nanoflares are impulsive energy releases by magnetic reconnection in the braided coronal magnetic field, which is a potential mechanism for heating the corona. However, there are s…
Constraints on Extragalactic Background Light using TeV Observations of BL Lacertae objects
Longhua Qin, Jiancheng Wang, Quangui Gao +5
The extragalactic background light (EBL) in the IR to UV bands partly absorbs very high energy (VHE, 100GeV) ray photons travelling over cosmological distances via pai…
New continuum and polarization observations of the Cygnus Loop with FAST II. Images and analyses
X. H. Sun, X. Y. Gao, W. Reich +4
We present total-intensity and polarized-intensity images of the Cygnus Loop supernova remnant (SNR) observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). T…
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- X. Chemical differentiation among the massive cores in G9.62+0.19
Y. P. Peng, T. Liu, S. -L. Qin +23
Investigating the physical and chemical structures of massive star-forming regions is critical for understanding the formation and the early evolution of massive stars. We performe…
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using CHCN, CHOCHO and CHOH lines
Sheng-Li Qin, Tie Liu, Xunchuan Liu +29
Hot cores characterized by rich lines of complex organic molecules are considered as ideal sites for investigating the physical and chemical environments of massive star formation.…