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M33 X-7:
Heaviest Stellar Black Hole Discovered in Nearby Galaxy

M33 X-7
Credit: Illustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/CfA/P.Plucinsky et al.; Optical: NASA/STScI/SDSU/J.Orosz et al.
JPEG (223.8 kb) Tiff (18.6 MB) PS (6 MB)

The main component of this graphic is an artist's representation of M33 X-7, a binary system in the nearby galaxy M33. In this system, a black hole is revolving around a star about 70 times more massive than the Sun (large blue object). This black hole is almost 16 times the Sun's mass, a record for black holes created from the collapse of a giant star. Other black holes at the centers of galaxies are much more massive, but this object is the record-setter for a so-called "stellar mass" black hole.

Chandra X-ray
Chandra X-ray of M33 X-7
In the illustration, an orange disk surrounds the black hole. This depicts material, fed by a wind from the blue companion star, which has been swept into orbit around the black hole. Rather than flowing unimpeded and uniformly into space, wind from the star is pulled towards the black hole by its powerful gravity. The wind that does make it past the black hole is disrupted, causing turbulence and ripples beyond the disk. The companion star itself is also distorted by the gravity from the black hole. The star is stretched slightly in the direction of the black hole, causing it to become less dense in this region and to appear darker.

M33 X-7Animations
M33 X-7 Animations
The inset shows a composite of data from NASA's Chandra X-ray Observatory (blue) and the Hubble Space Telescope. The bright objects in the inset image are young, massive stars around M33 X-7, and the bright, blue Chandra source is M33 X-7 itself. X-rays from Chandra reveals how long the black hole is eclipsed by the companion star, which indicates the size of the companion. Observations by the Gemini telescope on Mauna Kea, Hawaii track the orbital motion of the companion around the black hole, giving information about the mass of the two members of the binary. Other observed properties of the binary were also used to help constrain the mass estimates of both the black hole and its companion.

Fast Facts for M33 X-7:
Credit  Illustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/CfA/P.Plucinsky et al.; Optical: NASA/STScI/SDSU/J.Orosz et al.
Scale  Inset image is 30 arcsec across
Category  Black Holes, Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 1h 33m 34.12s | Dec +30d 32m 11.6°
Constellation  Triangulum
Observation Date  12 pointings between Sept 21-Nov 26, 2005
Observation Time  114 hours
Obs. ID  6378, 6382, 6384, 6386, 7170-7171, 7196-7197, 7199, 7208, 7226
Color Code  X-ray (blue)
Instrument  ACIS
References Orosz, J.A. et al. 2007, Nature, 449, 872
Distance Estimate  About 2.6 million light years from Earth
Release Date  October 17, 2007

More Information on M33 X-7:
Press Room: M33 X-7 Press Release
More Images of M33 X-7
M33 X-7 Animations
M33 X-7 Handout: html | pdf
Powerpoint and PDF
Chandra Chronicles: Solving the 26 Year Old Puzzle of M33 X-7
Related Chandra Images:
Photo Album: Bootes Field (12 Mar 07)
Photo Album: Black Hole Inside a Globular Star Cluster (07 Jan 07)
Photo Album: GOODS Chandra Deep Field South (01 Jun 04)
Photo Album: Cygnus X-1, XTE J1650-500 & GX 339-4 (17 Sep 03)
More Information on Black Holes:
X-ray Astronomy Field Guide: Black Holes
Questions and Answers: Black Holes
Chandra Images: Black Holes
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


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