M87 Radio Halo |
 | Minimum credit line: Image courtesy of NRAO/AUI
and F.N. Owen, J.A. Eilek and N.E. Kassim(for details, see .
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This is a VLA image of the galaxy M87, showing details of the large-scale, radio-emitting "bubbles" believed to be powered by the black hole at the galaxy's center. The galaxy's center (and the black hole) lie deep within the bright, reddish region in this image. The structure in this image is approximately 200,000 light-years across. This image was made at a radio wavelength of 90 centimeters.
Investigator(s): F. Owen, J. Eilek, and N. Kassim This image is available in the following downloadable versions:
- 480 x 496
- 900 x 930
- 2147 x 2219
If you would like to obtain a higher resolution version of this image,
please contact .
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Telescope
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VLA
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Date of Observation
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1999-00-00
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Type of Observation
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Continuum Observations
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Band
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P
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Wavelength
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90 cm
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Frequency
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330 MHz
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Center of Image
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RA: 12:30:49.42, Dec: 12:23:28.00 (J2000)
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Field of View
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0.2500 x 0.2500 degrees
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Technical Caption
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The convolving beam for this maximum entropy image
is 7.8"x6.2", P.A.=86deg.
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- Astronomical database entries for M87
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