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Encyclopedia > Radio galaxy

An active galaxy is a galaxy where a significant fraction of the energy output is not emitted by the normal components of a galaxy: stars, dust and interstellar gas. This energy, depending on the active galaxy type, can be emitted across most of the electromagnetic spectrum, as infrared, radio waves, UV, X-ray and gamma rays.

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A 5000 light-year (50 Em or 30,000,000,000,000,000 mile) long jet is ejected from active galaxy M87 (the yellow ball at top left). Electrons are ejected outward at near light-speed, emitting eerie blue light.

Frequently, the abbreviation AGN (Active Galactic Nuclei) is used, since all active galaxies appear to be powered by a compact region in the galactic centre. Some of these compact regions emit jets of matter that can extend for very large distances, powering extended structures (such as radio galaxies and radio-loud quasars). But in all cases the active nucleus or central engine is the fundamental source of energy.


The standard theoretical model is that the energy is generated by matter falling onto a supermassive black hole of between 106 and 109 solar masses. As the material falls into the black hole, angular momentum causes the material to flatten into an accretion disk. Frictional heating causes the infalling material to turn into plasma, and this charged moving material produces a strong magnetic field via the alpha mechanism. Frequently, one observes jets emanating from the accretion disk, although the mechanism of formation of those jets is poorly understood. The accretion mechanism is highly efficient at turning matter into energy, and can convert almost 50% of the mass-energy of an object into energy as compared with only a few percent with nuclear fusion.


It is believed that when the black hole has eaten all of the gas and dust in its neighborhood that the active galactic nucleus ceases to emit large amounts of radiation and becomes a normal galaxy. This model is supported by what appears to be a quiet supermassive black hole in the center of the Milky Way, and in other nearby galaxies, and also nicely explains why quasars appear to have been much more common in the early universe, when more fuel was available.


This model also explains the different types of active galactic nuclei, which are believed to all be due to the same type of source, but can appear quite different depending on the angle the source makes to the earth, and the amount of gas and dust available to be fed into the black hole.


Types of active galaxies

Seyferts, quasars and blazars are the main types of AGNs that emit high-energy radiation (X-rays). Quasars, in particular, are thought to be the most consistently luminous objects in the known universe.


Radio galaxies are a heterogeneous group of radio-emitting objects. Most of them have huge symmetrical lobes from which the greater part of the radio emission comes. Some of them show a jet or jets (the most famous example being the giant galaxy M87 in the Virgo cluster) coming directly from the nucleus and going to the lobes. The jets are believed to be the visible manifestations of the beam of high-energy particles that power the lobes. The radio emission is synchrotron radiation, implying that the radio lobes and jets contain relativistic electrons and magnetic fields.


Some of the different types of active galaxy are linked by Unified models in which they are really the same class of object seen at different viewing angles, with relativistic beaming and dust obscuration causing the observational differences. The two main unified models link the different classes of Seyferts and radio galaxies, quasars and blazars.


See also: Quasar, Seyfert galaxy, Blazar, Black hole.


  Results from FactBites:
 
Radio astronomy - Wikipedia, the free encyclopedia (917 words)
Radio astronomy is the study of celestial phenomena through measurement of the characteristics of radio waves emitted by physical processes occurring in space.
A 151 MHz map of the region: 140° to 180° galactic longitude; -5° to 5° galactic latitude from the CLFST at the Mullard Radio Astronomy Observatory.
Radio astronomy is also partly responsible for the idea that dark matter is an important component of our universe; radio measurements of the rotation of galaxies suggest that there is much more mass in galaxies than has been directly observed (see Vera Rubin).
Most distant group of galaxies known in the universe (1181 words)
The radio galaxies are amongst the most massive objects in the early Universe and there has long been circumstantial evidence that they are located at the heart of young clusters of galaxies, still in the process of formation.
Radio galaxies are therefore potential beacons for pinpointing regions of the Universe in which large galaxies and clusters of galaxies are being formed.
To search for galaxies at the same distance as the radio galaxy, the pictures were optimised in sensitivity for the sharp colour emitted by glowing hydrogen gas at the distance of the radio galaxy [2].
  More results at FactBites »

 
 

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