Skip to main content

ORIGIN OF RADIO EMISSION IN RADIO-QUIET QUASARS

Image Credit: NASA/Goddard Space Flight Center

Radio emission of radio-quiet quasars may be due to stars formation in the quasar host galaxy, to a jet launched by the supermassive black hole, or to relativistic particles accelerated in a wide-angle radiatively-driven outflow.


Recently some authors (Zakamska et al 2016) examine whether radio emission from radio-quiet quasars is a byproduct of stair formation in their hosts. They find that even the most generously computed star formation rates are insufficient to explain the observed radio emission, by about an order of magnitude. They cannot distinguish between radio emission due to compact weak jets and radio emission due to wide angle winds. The problem of distinguishing radio emission from compact jets from radio emission as a bi-product of radiatively driven has proven espexially difficult because the two mechanisms are similar in terms of energetics.


Read more>>
http://arxiv.org/pdf/1511.00013v2.pdf
http://mnras.oxfordjournals.org/content/455/4/4191.abstract

Labels

Etichette:

Comments

Post a Comment

Popular posts from this blog

ORBITAL PERIODS OF THE PLANETS

For orbital period generally we refer to the sidereal period, that is the temporal cycle that it takes an object to make a full orbit, relative to the stars. This is the orbital period in an inertial (non-rotating) frame of reference (365,25 days for the earth).
Post a Comment
Read more

THE HITCHCHIKER'S GUIDE TO THE LOCAL SUPERCLUSTER

Image: Virgo Supercluster. Credit: Andrew Z. Colvin The Virgo Supercluster is a region with a diameter of 33 megaparsecs (~1000 times larger the Milky Way's diameter) containing at least 100 galaxy groups and clusters.
Post a Comment
Read more

MILLISECOND PULSAR ORIGIN OF THE GALACTIC CENTER GEV EXCESS

Image: The Milky Way. Credit: Serge Brunier Using γ-ray data from the Fermi Large Area Telescope, various groups have identified a clear excess emission in the inner Galaxy, at energies around a few GeV. This excess attracted great attention, because it has properties typical for a dark matter annihilation signal.
Post a Comment
Read more