ESA’s XMM-Newton X-ray space observatory has found a wind of high-speed gas streaming from the centre of a bright spiral galaxy like our own that may be reducing its ability to produce new stars. The Seyfert galaxy, known as IRAS17020+4544 and located 800 million light-years from Earth, has a supermassive black hole at its core with a mass of nearly six million Suns.
A team of astronomers has found an enigmatic gas cloud, called CO-0.40-0.22, only 200 light-years away from the centre of the Milky Way. The cloud contains gas with a very wide range of speeds. The so-called velocity dispersion is best explained by the gravitational attraction of an intermediate mass black hole. If that is the case, then this is the first detection of such a body.
In this season of post-Christmas gym memberships, black holes have shown that they too can lose a lot of the weight of the stars that surround them. One unusually star-deprived black hole at the site of two merged galaxies could provide new insight into black hole evolution and behaviour, according to observations with the Hubble Space Telescope and Chandra X-ray Observatory.
Supermassive black holes at the centres of galaxies can spawn tremendous bipolar jets extending over hundreds of thousands of light-years. A CfA study of the bright radio jet galaxy Pictoris suggests that bright X-ray emission from the jets is produced by rapidly moving charged particles in magnetic fields.
There may be fewer pairs of supermassive black holes orbiting each other at the cores of giant galaxies than previously thought, according to a new study. When two massive galaxies harbouring supermassive black holes collide, their black holes ultimately combine — a process that could be the strongest source of elusive gravitational waves, still yet to be directly detected.