Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars
High Energy Astrophysical Phenomena
2015-06-11 v1
Abstract
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.
Keywords
Cite
@article{arxiv.1210.5801,
title = {Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars},
author = {YuanJie Du and GuoJun Qiao},
journal= {arXiv preprint arXiv:1210.5801},
year = {2015}
}
Comments
Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 3 pages, 2 figures