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C153:
Too Fast, Too Furious: A Galaxy's Fatal Plunge

C153
Credit: X-ray: NASA/CXC/SAO/UMass/D.Wang et al.
Optical: NASA/STScI/U.Alabama/W.Keel
Radio: NRAO/ F.Owen
Optical (OII): Gemini Obs./M.Ledlow
JPEG (225.63 kb) Tiff (2.87 MB) PS (4.69 MB)
zoom Zoom into C153 (flash)

These images offer a dramatic look at C153, a galaxy being ripped apart as it races at 4.5 million miles per hour through a distant cluster of galaxies. The infalling galaxy's gas is being stripped by the pressure of 20-million-degree Celsius gas that permeates the cluster.

At left is a composite image made by combining the four images at right, taken in X-ray, radio, and visible wavelengths as well as the visible, green light emitted by oxygen ions. Long comet-like streamers of gas can be seen flowing from the galaxy as it travels through the cluster called Abell 2125. The images span about one million light years.

The Chandra X-ray image shows a tail of hot gas extending from C153. The temperature of the gas tail is about 10 million degrees Celsius, cooler than the surrounding cluster gas. This temperature difference is further evidence that gas is being stripped from the galaxy. The image taken in visible light from glowing oxygen ions shows a similar tail forming as gas with a temperature of about 10,000 degrees Celsius is pulled from the galaxy.

Hubble's broad band visible-light image reveals intricate detail in the distribution of stars and dust within C153. The galaxy exhibits evidence of a large-scale disturbance that has left its star-forming regions concentrated to one side of its disk and beyond. Dust features are twisted into chaotic patterns, obscuring any spiral pattern the galaxy once had.

Radio observations depict high-energy particles as they spiral through the galaxy's magnetic field, with some escaping in a perpendicular direction to the galaxy's disk. The high-energy particles probably came from a supermassive black hole.

Fast Facts for C153:
Credit  X-ray: NASA/CXC/SAO/UMass/D. Wang et al.
Optical: NASA/STScI/U. Alabama/W. Keel
Radio: NSF/NRAO/F. Owen
Optical [OII]: NSF/NOAO/KPNO/M.Ledlow
Scale  Each panel is 34 arcsec per side
Category  Normal Galaxies & Starburst Galaxies
Groups & Clusters of Galaxies
Coordinates (J2000)  RA 15h 41m 09.76s | Dec +66º 15' 45.00"
Constellation  Ursa Major/Draco
Observation Date  August 24, 2001
Observation Time  22 hours
Obs. ID  2207
Color Code  X-ray (purple), Optical (yellow), Radio (red), Optical [OII] (green)
Instrument  ACIS
Distance Estimate  3 billion light years (920 million parsecs)
Release Date  January 06, 2004

More Information on C153:
Press Room: C153 Press Release
More Images of C153
C153 Animations
C153 Handout: html | pdf
Zoom in on C153 (flash)
Powerpoint and PDF
Related Chandra Images:
Photo Album: Abell 2125 (13 Aug 04)
Photo Album: M86 (01 Oct 03)
Photo Album: NGC 4631 (19 Jul 01)
More Information on Normal Galaxies & Starburst Galaxies:
X-ray Astronomy Field Guide: Galaxies
Questions and Answers: Normal Galaxies & Starburst Galaxies
Chandra Images: Normal Galaxies & Starburst Galaxies
More Information on Groups & Clusters of Galaxies:
X-ray Astronomy Field Guide: Groups & Clusters of Galaxies
Questions and Answers: Galaxies, Galaxy Clusters, AGN, and Quasars
Chandra Images: Groups & Clusters of Galaxies


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