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| 天文和天体物理学研究(英文版) |
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| FQ: 月刊 |
| AD of Publication: 北京市 |
| Lanuage: 英文; |
| ISSN: 1674-4527 |
| CN: 11-5721/P |
| YP: 1981 |
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Url: 中国科学院国家天文台 |
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Recommended Journals |
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| 2013
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Catalog
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Testing Lorentz violation with binary pulsars:constraints on standard model extension |
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Yi Xie Department of Astronomy,Nanjing University,Nanjing 210093,China Key Laboratory of Modern Astronomy and Astrophysics,Nanjing University,Ministry of Education,Nanjing 210093,China | |
The spectral properties of Fermi blazars:the spectral sequence and unification of blazars |
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Luo-En Chen 1,Huai-Zhen Li 1,Ting-Feng Yi 2,Shu-Bai Zhou 3 and Kai-Yi Li 1 1 Physics Department,Yuxi Normal University,Yuxi 653100,China 2 Physics Department,Yunan Normal University,Kunming 650092,China 3 Physics Department,Yunan University,Kunming 650091,China | |
A multi-wavelength study of the gravitational lens COSMOS J095930+023427 |
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Shuo Cao 1,2,Giovanni Covone 2,3,Maurizio Paolillo 2,3 and Zong-Hong Zhu 1 1 Department of Astronomy,Beijing Normal University,Beijing 100875,China;2 Dipartimento di Scienze Fisiche,Universita` di Napoli "Federico II," Complesso Universitario di Monte S.Angelo,via Cinthia,80126 Napoli,Italy 3 INFN,Sezione di Napoli,Complesso Universitario di Monte S.Angelo,via Cinthia,80126 Napoli,Italy | |
A multi-transition molecular line study of infrared dark cloud G331.71+00.59 |
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Nai-Ping Yu and Jun-Jie Wang National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China;NAOC-TU Joint Center for Astrophysics,Lhasa 850000,China | |
~(12)CO J=2-1 and~(12)CO J=3-2 observations toward the high-mass protostellar candidate IRAS 20188+3928 |
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Jin-Long Xu and Jun-Jie Wang National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China;NAOC-TU Joint Center for Astrophysics,Lhasa 850000,China | |
Star formation associated with the infrared dust bubble N68 |
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Chuan-Peng Zhang 1,2,3 and Jun-Jie Wang 1,2 1 National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China;2 NAOC-TU Joint Center for Astrophysics,Lhasa 850000,China 3 University of Chinese Academy of Sciences,Beijing 100049,China | |
Delayed onset and fast rise of prompt optical-UV emission from gamma-ray bursts in molecular clouds |
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Xiao-Hong Cui 1,Zhuo Li 2,3 and Li-Ping Xin 1 1 National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China;2 Department of Astronomy,Peking University,Beijing 100871,China 3 Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China | |
The effects of viscosity on circumplanetary disks |
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De-Fu Bu 1,Hsien Shang 2 and Feng Yuan 1 1 Key Laboratory for Research in Galaxies and Cosmology,Shanghai Astronomical Observatories,Chinese Academy of Sciences,Shanghai 200030,China;2 Institute of Astronomy and Astrophysics,Academia Sinica (ASIAA) | |
Structure of ADAFs in a general large-scale B-field:the role of wind and thermal conduction |
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Amin Mosallanezhad 1,2,Mehdi Khajavi 3 and Shahram Abbassi 2,4 1 Center for Excellence in Astronomy & Astrophysics (CEAA-RIAAM),P.O.Box 55134-441,Maragha,Iran 2 School of Physics,Damghan University,P.O.Box 36715-364,Damghan,Iran 3 Department of Physics,School of Sciences,Ferdowsi University of Mashhad,Mashhad,91775-1436,Iran 4 School of Astronomy,Institute for Research in Fundamental Sciences,P.O.Box 19395-5531,Tehran,Iran | |
The neutrino energy loss by electron capture of nuclides ~(55)Co and ~(56)Ni in explosive stellar environments |
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Jing-Jing Liu College of Science and Technology,Qiongzhou University,Sanya 572022,China | |
Phase analysis of sunspot group numbers on both solar hemispheres |
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Lin-Hua Deng 1,2,Zhong-Quan Qu 1,Xiao-Li Yan 1 and Kai-Rang Wang 3 1 National Astronomical Observatories /Yunnan Astronomical Observatory,Chinese Academy of Sciences,Kunming 650011,China2 Graduate University of Chinese Academy of Sciences,Beijing 100049,China 3 North China Electric Power University,Beijing 102206,China | |
Concerning spikes in emission and absorption in the microwave range |
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Gennady P.Chernov 1,2,Robert A.Sych 1,3,Guang-Li Huang 4,Hai-Sheng Ji 4,Yi-Hua Yan 1 and Cheng-Ming Tan 1 1 Key Laboratory of Solar Activity,National Astronomical Observatory,Chinese Academy of Sciences,Beijing 100012,China2 Pushkov Institute of Terrestrial Magnetism,Ionosphere and Radio Wave Propagation,Russian Academy of Sciences (IZMIRAN),Troitsk,Moscow region,142190,Russia 3 Institute of Solar-Terrestrial Physics,126,Lermontov St.,Irkutsk,Russia 4 Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China |
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