Multiwavelength Emission from Blazars - Conference Summary

Details Multiwavelength Emission from Blazars - Conference Summary Multiwavelength Emission from Blazars - Conference Summary

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..341u&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 341-349

Computer Science

Graphics

1

Blazars, Spectral Energy Distributions, Gamma-Ray Emission, Radio Emission, Host Galaxies, Blazar Demographics, Redshifts, Polarization, Yung Wing, Optical Emissions, Emission Mechanism, Black Holes

Scientific paper

Presentations at the Guangzhou Conference on Multiwavelength Emission from Blazars confirmed our understanding of blazars as relativistic jets closely aligned with the line of sight. Powerful new studies have been enabled by the Fermi gamma-ray satellite and new groundbased TeV facilities, which are an order of magnitude more sensitive than their predecessors. Combining gamma-ray data with VLBA radio and with optical/IR photometry has shed new light on the emission mechanisms and the jet geometry. This conference summary sets the context for the 4th blazar conference and presents some of the highlights from the meeting, as well as the questions that remain outstanding.

Affiliated with

Also associated with

No associations

Rating

Multiwavelength Emission from Blazars - Conference Summary does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multiwavelength Emission from Blazars - Conference Summary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength Emission from Blazars - Conference Summary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-919732