| dc.contributor.author | Zacharias, Michael | |
| dc.date.accessioned | 2019-09-11T05:44:09Z | |
| dc.date.available | 2019-09-11T05:44:09Z | |
| dc.date.issued | 2018 | |
| dc.identifier.citation | Zacharias, M. 2018. Blazar variability -- expect the unexpected. High Energy Astrophysics in Southern Africa (HEASA2018), 1-3 Aug, Parys, South Africa. Proceedings of science, 33: Article no 33. [https://doi.org/10.22323/1.338.0033] | en_US |
| dc.identifier.issn | 1824-8039 (Online) | |
| dc.identifier.uri | http://hdl.handle.net/10394/33305 | |
| dc.identifier.uri | https://pos.sissa.it/338/033/pdf | |
| dc.identifier.uri | https://doi.org/10.22323/1.338.0033 | |
| dc.description.abstract | Despite significant progress in both data taking and the development of theory, blazars keep offering surprises. While many frequency bands are now covered by long-term monitoring efforts on at least a few selected sources, blazars remain unpredictable and the same source may exhibit vastly different behaviors. Here, an overview is given about four selected sources, namely 3C\,279, PKS\,2155-304, PKS\,1510-089 and CTA\,102. All of them exhibited, indeed, highly unexpected events | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Sissa Medialab | en_US |
| dc.title | Blazar variability -- expect the unexpected | en_US |
| dc.type | Presentation | en_US |
| dc.contributor.researchID | 29092086 - Zacharias, Michael | |
