Title | The 3-D trajectories of pulsars in the Galaxy |
Authors | Wei, Ying-Chun Wu, Xin-Ji Peng, Qiu-He Wang, Na |
Affiliation | Chinese Acad Sci, Natl Astron Observ, Urumqi Observ, Urumqi 830011, Peoples R China. Peking Univ, Dept Astron, Beijing 100871, Peoples R China. Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China. |
Keywords | pulsars : general stars : kinematics stars : rotation VELOCITY DISTRIBUTION RADIO PULSARS |
Issue Date | 2006 |
Citation | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS.6(291-293). |
Abstract | Based on the undisturbed finitely thick disk gravitational potential, 3-D trajectories of pulsars are followed with initial locations and velocities randomly selected from a model distribution. Three typical instances are followed for some 10(11) yr, and their Poincare sections are used as diagnostics of their motion. We find that the vertical-to-parallel range ratio (relative to the Galactic plane) to be an important parameter: as this ratio increases, the pulsar's motion changes from being regular to being irregular/chaotic. |
URI | http://hdl.handle.net/20.500.11897/399563 |
ISSN | 1009-9271 |
Indexed | SCI(E) CPCI-S(ISTP) |
Appears in Collections: | 物理学院 |