Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

Autor:	Du, YuanJie, Qiao, GuoJun
Rok vydání:	2012
Předmět:	Astrophysics - High Energy Astrophysical Phenomena
Druh dokumentu:	Working Paper
DOI:	10.1017/S1743921312024180
Popis:	The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish our single magnetic pole model from two-pole models (e.g. outer gap model and two-pole caustic model), the convincing values of the magnetic inclination angle and the viewing angle will play a key role. Comment: Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 3 pages, 2 figures
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1210.5801 Zobrazit plný text záznamu View this record from Arxiv