File:Crab-pulsar hi.tif
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Summary
[edit]DescriptionCrab-pulsar hi.tif |
The Crab Nebula (M1) About this Image The Crab Nebula is a remnant of the supernova observed by Chinese, Japanese, and possibly natives of the southwest of the U.S.A. in 1054 AD. This image of the Crab shows the 33 millisecond pulsar as a bright point source near the center. Investigator(s): T. Velusamy
Visit related website http://images.nrao.edu/Galactic_Sources/Supernova_Remnants/34
Telescope VLA Date of Observation 1990-00-00 Type of Observation Continuum Observations Center of Image RA: 05:34:31.97, Dec: 22:00:52.10 (J2000) Field of View 0.3333 x 0.3333 degreesTechnical Caption VLA in A B D configuration using 27 antennas. |
Source | http://images.nrao.edu/335 http://images.nrao.edu/images/Crab-pulsar_hi.tif |
Author | Minimum credit line: Image courtesy of NRAO/AUI (for details, see Image Use Policy). |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:15, 19 February 2017 | ![]() | 2,308 × 1,882 (12.43 MB) | Fabian RRRR (talk | contribs) | == {{int:filedesc}} == {{Information |Description=The Crab Nebula (M1) About this Image The Crab Nebula is a remnant of the supernova observed by Chinese, Japanese, and possibly natives of the southwest of the U.S.A. in 1054 AD. This image of the Cra... |
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Width | 2,308 px |
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Height | 1,882 px |
Bits per component |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 2 |
Horizontal resolution | 118.11023712158 dpc |
Vertical resolution | 118.11023712158 dpc |
Data arrangement | chunky format |