Modelling Neutral Hydrogen Discs of Spiral Galaxies
参考文献14
-
1Zou Z L and Hart J L 2000 Chin. Phys. Lett. 17 935
-
2Corbelli E and Salpeter E E 1993 Astrophys. J. 419 104
-
3Dove J B and Shull J M 1994 Astrophys. J. 423 196
-
4Maloney P 1992 Astrophys. J. 398 L89
-
5Maloney P 1993 Astrophys. J. 414 41
-
6Hoffman G L, Lu N Y, Salpeter E E, Farhat B, Lamphier C and Roos T 1993 Astron. J. 106 39
-
7Linder S M 1998 Astrophys. J. 495 637
-
8Lin W P, BSrner G and Mo H J 2000 Mon. Not. R. Astron.Soc. 319 517
-
9Ferland G J 1996 Hazy, a Brief Introduction to Cloudy(University of Kentucky,Department of Physics and Astronomy Internal Report)
-
10Sofue Yet al 1999 Astrophys. J. 523 136
-
1Jun Ma (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012) E-mail:majun@vega.bac.pku.edu.cn.A Method of Obtaining the Pitch Angle of Spiral Arms and the Inclination of Galactic Discs[J].Chinese Journal of Astronomy and Astrophysics,2001,1(5):395-405.
-
2XU Zhou1,2 & WEI DaMing1,3 1 Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China,2 Graduate University of Chinese Academy of Sciences, Beijing 100012, China,3 Joint Center for Particle Nuclear Physics and Cosmology of Purple Mountain Observatory-Nanjing University, Nanjing 210008, China.The red damping wing of Gunn-Peterson trough in the high redshift GRBs[J].Science China(Physics,Mechanics & Astronomy),2009,52(9):1428-1433.
-
3Jun MaNational Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012.Vertical Scale Parameter Estimates for 48 Non-edge-on Spiral Galaxies[J].Chinese Journal of Astronomy and Astrophysics,2003,3(6):499-504.
-
4Wei-Peng Lin and Zhen-Long Zou ( Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012,CAS-Peking University Joint Beijing Astrophysical Center, Beijing 100871,Shanghai Astronomical Observatory,the Partner Group of MPI fur Astrop.Origin and Properties of Strong MgII Quasar Absorption Line Systems[J].Chinese Journal of Astronomy and Astrophysics,2001,1(1):21-28.
-
5B. Drz■z'la.Application of continuous spectra of radii of influence and some other possibilities of generalisation of subsidence trough description[J].中国有色金属学会会刊：英文版,2005,15(S1):269-271.
-
6Yang Chen,Yu Bai,Xiang-Tao He,Jiang-Hua Wu,Jing Wang,Qing-Kang Li,Yan-Chun Sun,Richard F. Green,Wolfgang Voges.The Multi-Wavelength Quasar Survey IV. Quasars in the Leo Cluster[J].Chinese Journal of Astronomy and Astrophysics,2007,7(4):595-600.
-
7Yu Bai,Yang Chen,Xiang-Tao He,Jiang-Hua Wu,Qing-Kang Li,Richard F.Green,Wolfgang Voges.The Multi-Wavelength Quasar Survey III. Quasars in Field 836[J].Chinese Journal of Astronomy and Astrophysics,2007,7(3):375-379.
-
8Purnima Srivastava.Largest Ediacaran discs from the Jodhpur Sandstone, Marwar Supergroup, India: Their palaeobiological significance[J].Geoscience Frontiers,2014,5(2):183-191. 被引量：1
-
9Kenji Mochizuki mochi@ astro. isas. ac. jp,The Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan..〔C II〕Continuum Intensity Ratio in the Far-Infrared Toward the Central Kiloparsec of the Nearby Spiral Galaxy M31[J].天文研究与技术,1999(S1):354-357.
-
10Proposal to construct a five hundred meter aperture (active) spherical telescope (FAST)[J].Chinese Science Bulletin,1998,43(15):1319-1320.
