Planetary Nebula NGC 7027

Minimum credit line: Image courtesy of NRAO/AUI (for details, see Image Use Policy).

About this Image

In 1977, the newly functioning VLA was used to map the radio emission from shells of hot gas, known as planetary nebulae, ejected from dying stars. The intensity of the radiation is denoted by color, which ranges from red (brightest) to blue (faintest). The effective angular size of the array's beam is shown in the inset. NGC 7027 represents one of the strongest and most unusual of the planetary nebulae.

Investigator(s):  R.M. Hjellming, R.C. Bignell, and B. Balick

Alternate Resolutions Help

This image is available in the following downloadable versions:If you would like to obtain a higher resolution version of this image, please contact us.

For More Information

Technical Data

    Telescope VLA 
    Date of Observation 1977-07-00 
    Type of Observation Continuum Observations 
    Band C 
    Wavelength 6 cm 
    Frequency 5.0 GHz 
    Center of Image RA: 21:07:1.59, Dec: 42:14:10.20 (J2000)  
    Field of View 0.0083 x 0.0083 degrees  
    Technical Caption VLA in hybrid-configuration using 6 antennas. Resolution 1.5 x 3.0 arcsec.  

  • Astronomical database entries for ngc7027
    • Query SIMBAD for more ngc7027 data


To search the Image Gallery for other images of ngc7027, click the Submit button.
Object Name Show Results As:

To search the Image Gallery for similar images, click the Submit button.
Category Sub-Category Telescope Mode Show Results As:

For more search options, please use our Advanced Search form.