The Chandra X-ray telescope continues to find some of the strangest objects in the Universe. Case in point - A pair of super massive black holes in the center of the spiral galaxy NGC 3393.
In the image here, we see a composite of blue which is the X-ray information from Chandra and gold which is the optical data from the Hubble Space Telescope. And according to the Wired article, the insert is just data of the high energy x-rays as seen by Chandra. The blue indicates hot gas but low x-ray energy, it also indicates strong iron bands which means the pair are growing.
Since black holes of this size are found mostly in the center of galaxies, the pair indicates a collision between two separate galaxies which also accounts for the large amount of gas and dust that are obscuring the pair.
What is truly amazing is that it is obvious that the pair of super-massive black holes are strongly influencing each other. Astronomically speaking they are close, but the influence is being felt over a distance of 490 light years! Plus at 160 million light years, they are the closest pair of super-massive black holes us.
In the image here, we see a composite of blue which is the X-ray information from Chandra and gold which is the optical data from the Hubble Space Telescope. And according to the Wired article, the insert is just data of the high energy x-rays as seen by Chandra. The blue indicates hot gas but low x-ray energy, it also indicates strong iron bands which means the pair are growing.
Since black holes of this size are found mostly in the center of galaxies, the pair indicates a collision between two separate galaxies which also accounts for the large amount of gas and dust that are obscuring the pair.
What is truly amazing is that it is obvious that the pair of super-massive black holes are strongly influencing each other. Astronomically speaking they are close, but the influence is being felt over a distance of 490 light years! Plus at 160 million light years, they are the closest pair of super-massive black holes us.

