Mapping planetary nebulae with the VLA

Details Mapping planetary nebulae with the VLA Mapping planetary nebulae with the VLA

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978s%26t....56..199h&link_type=abstract

Sky and Telescope, vol. 56, Sept. 1978, p. 199, 200.

Astronomy and Astrophysics

Astronomy

4

Mapping, Planetary Nebulae, Radio Astronomy, Radio Telescopes, Astronomical Maps, Radio Sources (Astronomy), Very Large Array (Vla)

Scientific paper

High resolution maps of extended radio sources have already been made with the Very Large Array (VLA) telescope in western New Mexico (using up to seven completed antennas with a maximum separation of 5.2 km). Attention is given to observations of planetary nebulae because they are compact objects with high surface brightness and relatively simple structure. Specifically, four nebulae were chosen for study: NCG 40 in Cepheus, NCG 7027 in Cygnus, NCG 7354 in Cepheus, and IC 3568 in Camelopardalis. Each nebula is smaller than 45 seconds of arc and is in high declination.

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