A minority of quasars show strong radio emission, which originates from jets of matter moving close to the speed of light. When looked at down the jet, these appear as a blazar and often have regions that appear to move away from the center faster than the speed of light (superluminal expansion.) This is an optical trick due to the properties of special relativity. (via Modern Physics and Astronomy: QUASAR)
Quasars have all the same properties as active galaxies, but are more powerful: Their Radiation is ‘nonthermal’ (i.e. not due to a black body), and some (~10%) are observed to also have jets and lobes like those of radio galaxies that also carry significant (but poorly known) amounts of energy in the form of high energy (i.e. rapidly moving, close to the speed of light) particles (either electrons and protons or electrons and positrons). Quasars can be detected over the entire observable electromagnetic spectrum including radio, infrared, optical, ultraviolet, X-ray and even gamma rays. Most quasars are brightest in their rest-frame near-ultraviolet (near the 1216 angstrom (121.6 nm) Lyman-alpha emission line of hydrogen), but due to the tremendous redshifts of these sources, that peak luminosity has been observed as far to the red as 9000 angstroms (900 nm or 0.9 µm), in the near infrared. A minority of quasars show strong radio emission, which originates from jets of matter moving close to the speed of light. When looked at down the jet, these appear as a blazar and often have regions that appear to move away from the center faster than the speed of light (superluminal expansion). This is an optical trick due to the properties of special relativity. (via Science: Quasar)
As you might expect, there are also two types of blazars: BL Lacs and Radio Quasars. A lot of work has been done to see which type of radio galaxies produce these blazars. The emerging picture is that BL Lacs are FRI jets pointing at us, and Radio Quasars are FRII jets pointing at us. Furthermore, there are some good reasons that come from physics that this should be the case. (via When do you reject a theory? « Life, the Universe, and Everything.)
First light from FERMI. Credit: NASA / FERMI (via Tom’s Astronomy Blog » GLAST is Now FERMI)
From the NASA press release:
[…] A fourth bright spot in the LAT image lies some 7.1 billion light-years away, far beyond our galaxy. This is 3C 454.3 in Pegasus, a type of active galaxy called a blazar. It’s now undergoing a flaring episode that makes it especially bright. […]
Blazars are a subset of the Active Galactic Nuclei (AGN or active galaxies). This radio-loud extragalactic objects are optically violent variable quasars, flat-spectrum quasars, high polarized quasars, and BL Lacertae (BL Lac) type objects, which display extremely intense, broad and rapidly varing electromagnetic emission, from radio to gamma-rays in some case. This emission is thought to originate in a relativistic plasma jet which is probably to be powered and accelerated by a billion solar mass black hole in gravitational accretion. Blazars show intense, flat-spectrum radio-loud emission, and their relativistic jet point nearly straight toward us. The Compton Gamma-Ray Observatory-EGRET found that many blazars are intense gamma-ray sources. This has been one of the most exciting astrophysical discovery of past decade. They are called classic BL Lac type objects if the optical continuum emission dominates compared to any line emission.
Briefly a blazar, is an object thet have the following characteristics:
It appear optically point-like on the sky, i.e. not appear widespread like a galaxy or a nebula. Some blazars have nebulae around them (are fuzzy), but most of the light comes from a point source.
Their spectra appear to be smooth (i.e. no strong absorption lines that a star might have) and flatter than a star. These two properties by themselves would make them a quasar.
Their visible light is often partially polarized.
Their output in all wavelength bands varies more rapidly, and by a larger amount than a classical quasar, with a flare-like behaviour.
Many blazar emits a significant fraction of their radiation at energy above 100 MeV. Their flux is peaked in high bands around 10Mev-1Gev for the LBL (red-blazar) class, around 1GeV-100GeV for the HBL (blue-blazar) class and around 200Gev-1TeV for the few TeV-blazar.
Above: Quasar 1317+520; false color: X-ray image from Chandra X-ray Observatory;
contours: 5 GHz radio image from the Very Large Array. Click here for more details. (via Blazar Research at Boston University)
An artist’s conception of the blazar BL Lacertae at it spurts out jets of charged particles accelerated by corkscrew magnetic field lines. (via An Astromical Black Hole, Painting | The News is NowPublic.com)