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NGC 4258 (M106):
Mysterious Arms Revealed

NGC 4258
Credit: X-ray: NASA/CXC/Univ. of Maryland/A.S. Wilson et al.; Optical: Pal.Obs. DSS; IR: NASA/JPL-Caltech; VLA: NRAO/AUI/NSF
JPEG (246.4 kb), Tiff (42.9 MB), PS (7.2 MB)

A combination of space and ground-based observations, including X-ray data from Chandra, has helped reveal the nature of the so-called anomalous arms in the spiral galaxy NGC 4258 (also known as M106). These arms have been known for decades, but their origin remained mysterious to astronomers.
NGC X-ray Image
NGC 4258 X-ray Image


In visible (shown in gold) and infrared (red) light, two prominent arms emanate from the bright nucleus and spiral outward. These arms are dominated by young, bright stars, which light up the gas within the arms. But in radio (purple) and Chandra's X-ray (blue) images, two additional spiral arms are seen.

Click for high-resolution animation
Multiwavelength Animation of NGC 4258
By analyzing data from XMM-Newton, Spitzer, and Chandra, scientists have confirmed earlier suspicions that the ghostly arms represent regions of gas that are being violently heated by shock waves. Previously, some astronomers had suggested that the anomalous arms are jets of particles being ejected by a supermassive black hole in nucleus of NGC 4258. But radio observations at the Very Large Array later identified another pair of jets originating in the core.

However, the jets do heat the gas in their line of travel, forming an expanding cocoon. Because the jets lie close to M106's disk, the cocoon generates shock waves and heat the gas in the disk to millions of degrees, causing it to radiate brightly in X-rays and other wavelengths.

Fast Facts for NGC 4258:
Credit  X-ray: NASA/CXC/Univ. of Maryland/A.S. Wilson et al.; Optical: Pal.Obs. DSS; IR: NASA/JPL-Caltech; VLA: NRAO/AUI/NSF
Scale  Image is 9.2 x 7.5 arcmin.
Category  Normal Galaxies & Starburst Galaxies, Quasars & Active Galaxies
Coordinates (J2000)  RA 2h 19m 00s | Dec +47° 18' 00"
Constellation  Canes Venatici
Observation Date  Three pointings from April 17, 2000 to May 29, 2001
Observation Time  4 hours
Obs. ID  350, 1618, 2340
Color Code  X-ray (blue); Optical (gold); IR (red); Radio (purple)
Instrument  ACIS
Also Known As M106
References Yang, Li, Wilson, Reynolds, ApJ, May 10 issue; Chandra Observations and the Nature of the Anomalous Arms of NGC 4258 (M106). Wilson, A.S., Yang,Y., Cecil, G., 2001, ApJ, 560, 689W
Distance Estimate  About 25 million light years
Release Date  April 10, 2007

More Information on NGC 4258:
Press Room: NGC 4258 Press Release
More Images of NGC 4258
NGC 4258 Handout: html | pdf
Zoom in on NGC 4258 (flash)
NGC 4258 Animations
Powerpoint and PDF
Download image for your desktop
Print Gallery image of NGC 4258
Related Chandra Images:
Photo Album: Andromeda Galaxy (M31) (05 Jun 06)
Photo Album: NGC 1068 (09 Jul 03)
Photo Album: NGC 3079 (19 Feb 03)
Photo Album: NGC 4631 (19 Jul 01)
More Information on Normal Galaxies & Starburst Galaxies :
X-ray Astronomy Field Guide: Normal Galaxies & Starburst Galaxies
Questions and Answers: Normal Galaxies & Starburst Galaxies
Chandra Images: Normal Galaxies & Starburst Galaxies
More Information on Quasars & Active Galaxies:
X-ray Astronomy Field Guide: Quasars & Active Galaxies
Questions and Answers: Quasars & Active Galaxies
Chandra Images: Quasars & Active Galaxies


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