File:Crab-pulsar hi.tif

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Summary[edit]

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 Crab shows the 33 millisecond pulsar as a bright point source near the center.

Investigator(s): T. Velusamy


For More Information

   Visit related website http://images.nrao.edu/Galactic_Sources/Supernova_Remnants/34


Technical Data


   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 degrees  
Technical 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/TimeThumbnailDimensionsUserComment
current21:15, 19 February 2017Thumbnail for version as of 21:15, 19 February 20172,308 × 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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