(click on image to enlarge)
UGC 3478, located in the constellation Camelopardalis, is what is known as a Seyfert galaxy. This is a type of galaxy with an AGN at its core. Like all such ‘active galaxies’, the brightness that you see here hides a supermassive black hole at the centre of the galaxy. A disc of gas spirals into this black hole, and as the material crashes together and heats up it emits very strong radiation. The spectrum of this radiation includes hard X-ray emission, which clearly mark it out from the stars in the galaxy. Despite the strong brightness of the compact central region, we can still clearly see the disc of the galaxy around it, which is a defining factor of a Seyfert galaxy.
Many active galaxies are known to astronomers at vast distances from Earth, thanks to the great brightness of their nuclei highlighting them next to other, dimmer galaxies. At 128 million light-years from Earth, UGC 3478 is positively neighbourly to us. The data used to make this image come from a Hubble survey of nearby powerful AGNs identified by their output of relatively high-energy X-rays, like this one, which it is hoped can help astronomers to understand how the galaxies interact with the supermassive black holes at their hearts.
[Image Description: A spiral galaxy, with two glowing spiral arms. They are filled with thin lines of dark dust, and surrounded by a faint cloud. One arm stretches further from the galaxy than the other. The point at the centre of the spiral is particularly bright. It is on a black background, mostly empty, except for some distant galaxies and a few bright stars in the foreground.]
Credit: ESA/Hubble & NASA, M. Koss, A. Barth
