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Galaxies 2016, 4(3), 21; doi:10.3390/galaxies4030021

The Conference Blazars through Sharp Multi-Wavelength Eyes

1
Institute for Astrophysical Research, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA
2
Instituto de Astrofísica de Andalucía, CSIC, Apartado 3004, 18080, Granada, Spain
3
Astronomical Institute, St. Petersburg State University, Universitetskij Pr. 28, Petrodvorets, 198504 St. Petersburg, Russia
*
Author to whom correspondence should be addressed.
Academic Editor: Emilio Elizalde
Received: 30 August 2016 / Accepted: 31 August 2016 / Published: 1 September 2016
(This article belongs to the Special Issue Blazars through Sharp Multi-wavelength Eyes)
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Note: In lieu of an abstract, this is an excerpt from the first page.

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Blazars are active, galactic nuclei with jets of magnetized, high-energy plasma that flow outward from the center of the host galaxy at near-light speeds.[...] View Full-Text
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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Marscher, A.P.; Gómez, J.L.; Jorstad, S.G. The Conference Blazars through Sharp Multi-Wavelength Eyes. Galaxies 2016, 4, 21.

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