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NGC 6240, John Bozeman

NGC 6240

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NGC 6240, John Bozeman

NGC 6240

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Description

Scientists have used Chandra to make a detailed study of an enormous cloud of hot gas enveloping two large, colliding galaxies. This unusually large reservoir of gas contains as much mass as 10 billion Suns, spans about 300,000 light years, and radiates at a temperature of more than 7 million degrees Kelvin. This giant gas cloud, which scientists call a "halo," is located in the system called NGC 6240. Astronomers have long known that NGC 6240 is the site of the merger of two large spiral galaxies similar in size to our own Milky Way. Each galaxy contains a supermassive black hole at its center. The black holes are spiraling toward one another, and may eventually merge to form a larger black hole. Another consequence of the collision between the galaxies is that the gas contained in each individual galaxy has been violently stirred up. This caused a baby boom of new stars that has lasted for at least 200 million years. During this burst of stellar birth, some of the most massive stars raced through their evolution and exploded relatively quickly as supernovas.

NGC 6240 Chandra X-ray
NGC 6240 Hubble Optical - WFPC2 F435W (Blue)
NGC 6240 Hubble Optical - Synthetic (Green)
NGC 6240 Hubble Optical - WFPC2 F814W (Red)

Credit: X-ray: NASA/CXC/SAO/E.Nardini et al; Optical: NASA/STScI
Observation Date: 4 pointings between Jul 2001 and May 2011
Obs. ID: 1590, 6908, 6909, 12713
Image Release: NGC 6240: Colossal Hot Cloud Envelops Colliding Galaxies (30 Apr 2013)

Processed with FITS Liberator, PixInsight and Photoshop 2024.

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NGC 6240, John Bozeman