Microvariability in Blazars |
| |
Authors: | MR Deshpande UC Joshi KS Baliyan S Ganesh |
| |
Institution: | (1) Physical Research Laboratory, Navrangpura, Ahmedabad, 380 009, India |
| |
Abstract: | Optically violent variable quasars and BL Lac objects, which form a subclass of active galactic nuclei are termed as Blazars.
Blazars show high degree variation in their flux and polarization in a relatively shorter period of time. They are strong
radio sources with a non-stellar continuum. Most of the BL Lac objects do not show any emission lines though in some cases
very weak lines are observed. They harbour in elliptical galaxies. Some BL Lacs show superluminal motion indicating the flow
of matter at relativistic speeds close to the line of sight. It is likely that the enormous energy produced by these objects
may be due to a massive black hole with an accretion disc system. Some Blazars have been observed to detect short time variations
in their flux and polarization in the visual band. These studies are aimed at understanding the physical processes taking
place in the central engine. Detecting shorter period variations assumes significance as they impose restrictions on the total
volume from where the huge amount of energy is comming out. To date the recorded shortest period variation in visual band
is 6.3 min in OJ 287, a BL Lac object. Attempts are being made to detect shorter period variations, which pose observational
challenges. It is generally accepted that the central engine of AGN harbours a massive blackhole with an accretion disc surrounding
it.
This revised version was published online in July 2006 with corrections to the Cover Date. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|