Milli-arcsec structure of 3C 345

Details Milli-arcsec structure of 3C 345 Milli-arcsec structure of 3C 345

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...247..774c&link_type=abstract

Astrophysical Journal, Part 1, vol. 247, Aug. 1, 1981, p. 774-779.

Astronomy and Astrophysics

Astrophysics

27

Astronomical Models, Galactic Structure, Quasars, Variability, Very Long Base Interferometry, Angular Resolution, Computer Techniques, Data Reduction, Mapping, Visibility

Scientific paper

The quasar 3C 345 has been studied at eight epochs between 1977.56 and 1979.92 using very-long-baseline interferometry, alternating between frequencies of 10.65 and 5.01 GHz. Hybrid maps for each epoch show that the source comprises a bright, barely-resolved 'core' with an inverted spectrum, and an elongated region of emission extending approximately 5 milliarcsec from its western side. The position angle of this 'jet' changes systematically from P.A. approximately -85 deg close to the core to P.A. approximately -75 deg at a radius of 3 milliarcsec. Components within this 'jet' change in position and brightness with time, but they do not show clear indications of superluminal expansion. No emission is found on the eastern side of the core above a level of 5% of the peak brightness.

Affiliated with

Also associated with

No associations

Rating

Milli-arcsec structure of 3C 345 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 Milli-arcsec structure of 3C 345, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Milli-arcsec structure of 3C 345 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1744378