The milli-arcsecond structure of 3C 147 and 3C 380 determined by hybrid mapping with a five-station array

Details The milli-arcsecond structure of 3C 147 and 3C 380 determined by hybrid mapping with a five-station array The milli-arcsecond structure of 3C 147 and 3C 380 determined by hybrid mapping with a five-station array

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235...11r&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 1, 1980, p. 11-17.

Astronomy and Astrophysics

Astronomy

42

Astronomical Maps, Quasars, Radio Astronomy, Stellar Structure, Very Long Base Interferometry, Astronomical Models, Brightness Temperature, Extragalactic Radio Sources, Point Sources

Scientific paper

Hybrid maps of 3C 147 and 3C 380 have been made from VLBI observations at 1671 MHz on a five-station network. The amount of amplitude and closure phase data is roughly double that obtained on four station networks, making these the most accurate and detailed maps of the milli-arcsecond structure of quasars that have yet been made. The morphologies of the sources are discussed briefly in the context of the beam model.

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