Wright's and Vayner's research indicates that 3C 298 does not fall within this normal scaling relationship
between nearby galaxies and the supermassive black holes that lurk at their center.
Not exact matches
Vanessa McBride at the University of Southampton in the UK and her colleagues looked at X-rays arriving from the space
between two
nearby galaxies, the Large and Small Magellanic clouds.
In the
nearby Universe, there is a direct relationship — a constant ratio —
between the masses of the black holes and that of the central «bulges» of the
galaxies.
Both M81 and M101 were observed with the Far - Infrared Surveyor (FIS) aboard AKARI in four far - infrared bands at 65, 90, 14... ▽ More We assess the relationships
between the surface densities of the gas and star formation rate (SFR) within spiral arms of the
nearby late - type spiral
galaxies M81 and M101.
Abstract: We assess the relationships
between the surface densities of the gas and star formation rate (SFR) within spiral arms of the
nearby late - type spiral
galaxies M81 and M101.