Very long baseline interferometry observations of 3C 147 and 3C 286 at 329 megahertz

Details Very long baseline interferometry observations of 3C 147 and 3C 286 at 329 megahertz Very long baseline interferometry observations of 3C 147 and 3C 286 at 329 megahertz

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..707s&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Mar. 15, 1980, p. 707-713.

Astronomy and Astrophysics

Astrophysics

35

Quasars, Radio Spectra, Very Long Base Interferometry, Astronomical Maps, Halos, Plasma Jets, Radiant Flux Density, Spectrum Analysis

Scientific paper

Hybrid maps of two quasars, 3C 147 and 3C 286, made at 329 MHz from VLBI observations are presented. Both objects consist of an unresolved core; an extended, asymmetric jet; and an even larger, completely resolved, halo. For 3C 147 it is possible to decompose the spectrum into individual component spectra; at 329 MHz the core of 3C 147 is found to be strongly self-absorbed. For both sources, the spectral index decreases monotonically from core to jet to halo.

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