A Star in Making |
 | Minimum credit line: Image courtesy of NRAO/AUI
and Luis Zapata, UNAM/Harvard-Smithsonian CfA(for details, see .
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False color image of a star in making located in the Orion Nebula. The color represents the radio emission detected by the Very Large Array telescope using its most
extended configuration, and thus allowed to reach a spatial resolution of about 20 AU. This image reveals its protoplanetary disk observed edge-on (the strongest clump, that has a size comparable to of our solar system) together with its outflow, that is perpendicular to the disk (the two faint clumps).
In the right bottom corner is shown an artist's conception of this phenomenon.
Investigator(s): Luis A. Zapata, Luis F. Rodriguez and Paul, T.P. Ho This image is available in the following downloadable versions:
- 514 x 500
- 900 x 875
- 2161 x 2100
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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2004-11-04
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Type of Observation
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Continuum Observations
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Band
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Q
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Wavelength
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7 mm
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Frequency
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45 GHz
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Center of Image
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RA: 05:24:0.00, Dec: -5:35:13.50 (J2000)
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Field of View
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0.0167 x 0.0167 degrees
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Technical Caption
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This radio image was obtained from the project AZ154. In this project we mapped the OMC1 South region in the Orion nebula using the VLA in its "A" configuration at 7mm, getting thus an angular resolution of about 0.05".
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