Supernova Factory in Arp 299 |
 | Minimum credit line: Image courtesy of NRAO/AUI
and HST/STScI(for details, see .
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This image of the colliding galaxy pair Arp 299 (also known as NGC 3690/IC694) was
produced combining radio wavelength observations from the National Radio
Astronomy Observatory's Very Large Array with data from the Hubble Space
Telescope. Radio emission is shown as red, near-infrared emission as green,
and ultraviolet emission as blue.
This colliding pair is a region of vigorous star formation which has
been investigated in the past. Since 1990, four supernova explosions have
been seen optically in Arp 299. Observations with the NRAO's Very Large
Array (VLA) showed a region near the nucleus of one of the colliding
galaxies which had all the earmarks of prolific star formation.
Observations with the VLBA and the GBT in 2002 and 2003 led to the
discovery of 5 supernovae concentrated in this region.
Investigator(s): J. Ulvestad, S. Neff & S. Teng This image is available in the following downloadable versions:
- 529 x 473
- 894 x 800
- 2039 x 1823
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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2000-10-24
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Type of Observation
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Continuum Observations
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Band
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C
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Wavelength
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6 cm
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Frequency
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5.0 GHz
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Center of Image
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RA: 11:28:33.00, Dec: 58:33:58.00 (J2000)
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Field of View
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0.0142 x 0.0197 degrees
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Technical Caption
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The radio emission is continuum emission at a frequency of 5 GHz.
The near-infrarred/ultraviolet data are observations made with the Hubble Space Telescope,
obtained from the data archive at the STScI.
The near-infrared emission is from an HST/WFPC2 observation through
the F814 filter, and the ultraviolet emission is from an HST/WFPC2
observation through the F255+F300 filters.
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