Two ultra-compact dwarf galaxies with supermassive black holes discovered
Astronomers have published a study in the Astrophysical Journal wherein they describe discovery of what they believe are two ultra-compact dwarf galaxies with supermassive black holes at the center.
The two galaxies are not the first of their kinds because such black hole-harboring ultra-compact dwarf galaxy have been observed before three years.
According to team of astronomers led by Chris Ahn from University of Utah in the US, the dwarf galaxies may be remnants of massive galaxies that were ripped apart by larger galaxies and that black holes lurk at the centre of most of these objects, potentially doubling the number of supermassive black holes known in the universe. Ahn says they still don’t fully understand how these galaxies would have formed and evolved in their lifetime.
“Maybe a fraction of the centers of all galaxies are actually these compact galaxies stripped of their outer parts,” Ahn said.
The authors measured two ultra-compact dwarf galaxies, named VUCD3 and M59cO, that lie far beyond the spiral arms of our Milky Way, orbiting massive galaxies in the Virgo galaxy cluster.
They detected a supermassive black hole in both galaxies – VUCD3’s black hole has a mass equivalent to 4.4 million suns, making up about 13 per cent of the galaxy’s total mass, and M59cO’s black hole has a mass of 5.8 million suns, making up about 18 per cent of its total mass.
By comparison, the monstrous black hole at the centre of the Milky Way has a mass of four million suns, but makes up less than .01 per cent of the galaxy’s total mass.
“It’s pretty amazing when you really think about it. These ultra-compact dwarfs are around 0.1 per cent the size of the Milky Way, yet they host supermassive black holes that are bigger than the black hole at the center of our own galaxy,” Ahn said.
To calculate the ultra-compact dwarf galaxies’ mass, the astronomers measured the movement of the stars using the Gemini North telescope located on Mauna Kea volcano in Hawaii.