Computer Science
Scientific paper
May 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1437x&link_type=abstract
The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1437-1441 (1997).
Computer Science
Active And Peculiar Galaxies And Related Systems, Magnitudes And Colors, Luminosities, Quasars, Radio, Microwave
Scientific paper
We present VLBA observations of three gamma-ray bright blazars: 0235+164, 1633+382 (4C38.41) and 2230+114 (CTA102). 0235+164 was unresolved at 22 and 43 GHz during the period between Nov. 1993 and Aug. 1996. The brightness of the core varied significantly. 1633+382 (4C38.41) has a sharp leading edge in its jet. The jet edge moved approximately at a constant velocity of (9.9+/-0.7)h-1c between March 1994 and May 1995. The velocity is much faster than that of (6.1+/-1.1)h-1c measured by Barthel et al. (1995). This may indicate that a component is moving at a faster speed. 2230+114 (CTA 102) produced several new components between Feb. 1995 and Aug. 1996. These components moved at apparent velocities of (12-21)h-1c. The components at ~1.7 mas and ~8 mas seem to be stationary.
Marscher Alan P.
Wehrle Ann E.
Xu Wei-Wei
No associations
LandOfFree
VLBA monitoring of three gamma-ray bright blazars: AO 0235+164, 1633+382 (4C 38.41) & 2230+114 (CTA 102) 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 VLBA monitoring of three gamma-ray bright blazars: AO 0235+164, 1633+382 (4C 38.41) & 2230+114 (CTA 102), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBA monitoring of three gamma-ray bright blazars: AO 0235+164, 1633+382 (4C 38.41) & 2230+114 (CTA 102) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-835397