Decameter interferometry of 3C 134

Details Decameter interferometry of 3C 134 Decameter interferometry of 3C 134

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62...38m&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Jan.-Feb. 1985, p. 38-42) Soviet Astronomy (ISSN 0038-5301), vol. 29, Jan.-Feb. 1985, p. 23-

Astronomy and Astrophysics

Astronomy

Decametric Waves, Interferometry, Radio Sources (Astronomy), Brightness Distribution, Visibility

Scientific paper

Results are presented of the observation of the radio source 3C 134 made by means of the wide-band decameter radio interferometer URAN-1. It is shown that the angular structure of this object does not appreciably differ from its radio brightness distribution at meter and decimeter waves. The analysis of radio interferometric measurements performered in the band of 20 to 1425 MHz has permitted to estimate the angular size of the source, which at the 50 per cent intensity level has been found equal to 37arcsec±7arcsec.

Affiliated with

Also associated with

No associations

Rating

Decameter interferometry of 3C 134 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Decameter interferometry of 3C 134, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Decameter interferometry of 3C 134 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1591357