DRAGNs in the sky

September 9, 2014 by Brian Koberlein, One Universe at a Time
Credit: National Radio Astronomy Observatory

A radio galaxy is a galaxy that emits large amounts of radio waves. They were first discovered in the 1950s, but it wasn't until the 1960s when a technique known as aperture synthesis was developed that we could resolve the distribution of radio emissions within a radio galaxy. It then became clear that many radio galaxies had a double-lobed structure emanating from a galactic core. It was suggested that these Double Radio Sources Associated with Galactic Nuclei be known a DRAGNs, though the term has never really caught on.

We now know that these lobed radio sources are powered by a galaxy's supermassive black hole. When a supermassive black hole eats nearby gas, dust and stars, it is known as an (AGN). These active black holes cause some of the surrounding material to stream off at high speed as jets. The jets stream away from the at tremendous speed, and can collide with the intergalactic medium. This forms lobes of radio bright material, as can be seen in the image above.

We see this in our own galaxy, which is one of the ways we know the Milky Way contains a supermassive black hole (although we also have more direct evidence). With our own galaxy we can see these lobes from past activity, but at present the region around the Milky Way black hole is fairly quiet. So it seems that go through active and quiet periods. It is a pattern we see in other galaxies as well.

DRAGNs in the Sky
A 1965 radio map of our galaxy, showing the double lobed structure. Credit: M. Ryle et al

When they were first discovered, and DRAGNs were seen as a distinct phenomena, different from other objects such as quasars an blazars. We now know that they are all driven by a similar process, and that how they appear to us depends largely on our view of the galaxy. We still use various terminology for radio galaxies, quasars, and the like, but we now understand that the lines between different categories are fuzzy.

Explore further: Supermassive black hole blows molecular gas out of a galaxy at 1 million kilometres per hour

Source:: One Universe at a Time


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1 / 5 (3) Sep 09, 2014
Excuse me, but those are not lobes; it is a cross-section of a torus. If it were observed from above or below it would be a ring. Any observer looking at the torus edge-on will see the bi-lobate structure.

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