Pulsars in gamma rays: What Fermi is teaching us
Abstract
The 2nd Fermi-LAT pulsar catalog includes 117 γ-ray pulsars, of which roughly one third are millisecond pulsars (MSPs) while the remaining two thirds split evenly into young radio-loud and radio-quiet pulsars. Although this large population will enable future, detailed studies of emission mechanisms and the evolution of the underlying neutron star population, some nearly-universal properties are already clear and unequivocal. We discuss some of these aspects below, including the altitude of the γ-ray emission site, the shape of the γ-ray spectrum, and the implications of the latter for the radiation mechanism.
- Publication:
-
Neutron Stars and Pulsars: Challenges and Opportunities after 80 years
- Pub Date:
- March 2013
- DOI:
- arXiv:
- arXiv:1211.3726
- Bibcode:
- 2013IAUS..291..307K
- Keywords:
-
- pulsar: general;
- gamma rays: observations;
- radiation mechanisms: nonthermal;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.)