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Astronomy in the News

Mercury Spring 2011 Table of Contents


ring of black holes

This composite image of Arp 147, a pair of interacting galaxies located about 430 million light years from Earth, shows X-ray data from NASA's Chandra X-ray Observatory (pink) and optical data from the Hubble Space Telescope (red, green, blue). Image courtesy of X-ray: NASA / CXC / MIT, Optical: NASA / STScI.

Giant Ring of Black Holes

Chandra X-ray Center

Arp 147 contains the remnant of a spiral galaxy (right side of the image) that collided with the elliptical galaxy (left of center). This collision has produced an expanding wave of star formation that shows up as a blue ring containing an abundance of massive young stars. These stars race through their evolution in a few million years or less and explode as supernovas, leaving behind neutron stars and black holes.

A fraction of the neutron stars and black holes will have companion stars, and may become bright X-ray sources as they pull in matter from their companions. The nine X-ray sources scattered around the ring in Arp 147 are so bright that they must be black holes, with masses that are likely ten to twenty times that of the Sun.

An X-ray source is also detected in the nucleus of the red galaxy on the left and may be powered by a poorly fed supermassive black hole. This source is not obvious in the composite image but can easily be seen in the X-ray image. Other objects unrelated to Arp 147 are also visible: a foreground star in the lower left of the image and a background quasar as the pink source above and to the left of the red galaxy.

Infrared observations with NASA's Spitzer Space Telescope and ultraviolet observations with NASA's Galaxy Evolution Explorer (GALEX) have allowed estimates of the rate of star formation in the ring.

 


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