File:Ms0735 xray 420.jpg

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Ms0735_xray_420.jpg(420 × 420 pixels, file size: 41 KB, MIME type: image/jpeg)

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English: This Chandra image shows two vast cavities - each 600,000 light years in diameter - in the hot, X-ray emitting gas that pervades the galaxy cluster MS 0735.6+7421 (MS 0735 for short). Although the cavities contain very little hot gas, they are filled with a two-sided, elongated, magnetized bubble of extremely high-energy electrons that emit radio waves.

The cavities appear on opposite sides of a large galaxy at the center of the cluster, which indicates that a gigantic eruption produced by the galaxy's supermassive black hole created the structures. The magnitude of the eruption suggests that as a large amount of gas swirled rapidly toward the central black hole, it generated intense electromagnetic fields that ejected a fraction of the gas in the form of powerful jets of high-energy particles.

As these jets blasted through the galaxy into the surrounding multimillion degree intergalactic gas, they pushed the hot gas aside to create the cavities. The mass of the displaced gas equals about a trillion Suns, more than the mass of all the stars in the Milky Way.
Date
Source CHANDRA X-ray Observatory CXC Operated for NASA by SAO, url=http://chandra.harvard.edu/photo/2005/ms0735/
Author NASA/CXC/Ohio U./B.McNamara
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Image is 4.2 arcmin per side. RA 07h 41m 50.20s | Dec +74° 14' 51.00" Camelopardus Observation date: November 30, 2003. Ref: B. McNamara et al 2005, Nature

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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5 January 2005

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current23:28, 24 November 2009Thumbnail for version as of 23:28, 24 November 2009420 × 420 (41 KB)Marshallsumter{{Information |Description={{en|1=This Chandra image shows two vast cavities - each 600,000 light years in diameter - in the hot, X-ray emitting gas that pervades the galaxy cluster MS 0735.6+7421 (MS 0735 for short). Although the cavities contain very li

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