| dc.contributor.author | Venter, Christo | |
| dc.contributor.author | Harding, Alice K. | |
| dc.contributor.author | Grenier, Isabelle | |
| dc.date.accessioned | 2018-05-29T07:05:33Z | |
| dc.date.available | 2018-05-29T07:05:33Z | |
| dc.date.issued | 2017 | |
| dc.identifier.citation | Venter, C. et al. 2017. High-energy emission properties of pulsars. XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop 12-17 June, 2017 Palermo, Italy. Proceedings of science, 306: Article no 038. [https://pos.sissa.it/306/038/pdf] | en_US |
| dc.identifier.issn | 1824-8039 (Online) | |
| dc.identifier.uri | http://hdl.handle.net/10394/26925 | |
| dc.identifier.uri | https://pos.sissa.it/306/038/pdf | |
| dc.identifier.uri | https://pos.sissa.it/306/ | |
| dc.description.abstract | The sheer number of new γ-ray pulsar discoveries by the Fermi Large Area Telescope since 2008,
combined with the quality of new multi-frequency data, has caused a revolution in the field of
high-energy rotation-powered pulsars. These rapidly rotating neutron stars exhibit rich spectral
and temporal phenomenology, indicating that there are still many unsolved mysteries regarding
the magnetospheric conditions in these stars – even after 50 years of research! Indeed, 2017marks
the golden anniversary of the discovery of the first radio pulsar, and theorists and observers alike
are looking forward to another half-century of discovery, with many new experiments coming
online in the next decades. In this review paper, we will briefly summarise recent HE pulsar observations,
mention some theoretical models that provide a basic framework within which to make
sense of the varied measurements, and finally review some of the latest theoretical developments
in pulsar emission modelling | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | PoS | en_US |
| dc.title | High-energy emission properties of pulsars | en_US |
| dc.type | Presentation | en_US |
| dc.contributor.researchID | 12006653 - Venter, Christo | |
