ORION

作品数：287被引量：151H指数：7
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Revisit of GeV Gamma-Ray Emission from Orion B with the Fermi Large Area Telescope
《Research in Astronomy and Astrophysics》2024年第9期128-135,共8页Wei Zeng Xiao-Na Sun Rui-Zhi Yang Jia-Chun He Zhao-Dong Shi Ting-Ting Ge Yun-Feng Liang En-Wei Liang 
supported by National Key R&D Program of China(grant No.2023YFE0117200);the National Natural Science Foundation of China(NSFC,grant Nos.12133003,12103011);R-Z.Y.is supported by the NSFC under grants 11421303,12041305;Science and Technology Program of Guangxi(grant Nos.AD 21220075 and 2024GXNSFBA010375);the national youth thousand talents program in China。
We revisit the γ-ray emission above 300 Me V towards the massive star-forming region of Orion B by adopting14 yr observations with the Fermi Large Area Telescope and utilizing the updated software tools.The extended ...
关键词：(ISM:)cosmic rays gamma-rays:ISM (Galaxy:)open clusters and associations:individual(NGC 2023 NGC 2024 NGC 2068 and NGC 2071) 
Symmetry properties and widths of the filamentary structures in the Orion A giant molecular cloud
《Research in Astronomy and Astrophysics》2021年第8期23-45,共23页Yu-Qing Zheng Hong-Chi Wang Yue-Hui Ma Chong Li 
supported by National Key R&D Program of China (Grant 2017YFA0402701);Key Research Program of Frontier Sciences of CAS (Grant QYZDJ-SSW-SLH047);support by the National Natural Science Foundation of China (NSFC,Grant No.1973091);supports by the NSFC (Nos.11503086 and 11503087)。
We identify 225 filaments from an H2 column density map constructed using simultaneous 12CO,13CO and C18O(J=1-0) observations carried out as a part of the Milky Way Imaging Scroll Painting(MWISP) project.We select 46 ...
关键词：ISM:clouds ISM:individual objects(Orion A) ISM:structure stars:formation 
The column density structure of Orion A depicted by N-PDF被引量：1
《Research in Astronomy and Astrophysics》2020年第4期139-155,共17页Yue-Hui Ma Hong-Chi Wang Chong Li Ji Yang 
supported by National Key R&D Program of China(2017YFA0402701);Key Research Program of Frontier Sciences of CAS(QYZDJSSW-SLH047);supports by the National Natural Science Foundation of China(Grant Nos.11503086 and 11503087)。
We have conducted a large-field simultaneous survey of 12 CO,13 CO and C18O J=1-0 emission toward the Orion A giant molecular cloud(GMC)with a sky coverage of4.4 deg2 using the Purple Mountain Observatory(PMO)-13.7 m ...
关键词：ISM:clouds ISM:individual objects(Orion A) ISM:structure stars:formation surveys TURBULENCE 
Photometric investigation of the K-type extremely shallow contact binary V1799 Orion
《Research in Astronomy and Astrophysics》2014年第9期1157-1165,共9页Nian-Ping Liu Sheng-Bang Qian Wen-Ping Liao Jia-Jia He Er-Gang Zhao Liang Liu 
Supported by the National Natural Science Foundation of China
New multi-color light curves of the very short period K-type eclipsing binary V1799 Ori were obtained and analyzed with the Wilson-Devinney code. The photometric solutions reveal that the system is a W-type shallow-co...
关键词：binaries： close -- binaries： eclipsing -- stars： individual （V1799 Off） 
C_2H, HC_3N and HNC observations in OMC-2/3
《Research in Astronomy and Astrophysics》2011年第6期671-678,共8页Qiang Liu Ji Yang Yan Sun Ye Xu 
supported by the National Natural Science Foundation of China (Grant Nos. 11003046, 11073054, 10733030 and 10621303);the National Basic Research Program of China (973 Program, Grant 2007CB815403)
For the first time, the OMC-2/3 region was mapped in C2H （1–0）, HC3N （10–9） and HNC （1–0） lines. In general, the emissions from all the three molecular species reveal an extended filamentary structure. The di...
关键词：ISM： abundances-ISM： individual （Orion Molecular Clouds）-ISM： molecules-stars： formation 
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