On the Superluminal Motion of Radio-Loud AGNs

Details On the Superluminal Motion of Radio-Loud AGNs On the Superluminal Motion of Radio-Loud AGNs

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..247z&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 247-249

Astronomy and Astrophysics

Astrophysics

Galaxies: Active, Galaxies: Jets, Radio Continuum: Galaxies, Radiation Mechanisms: Non-Thermal, Quasars: General., Galaxies: Active—Galaxies: Jets—Radio Continuum: Galaxies—Radiation Mechanisms: Non-Thermal—Quasars: General.

Scientific paper

Apparent superluminal motion of different radio-loud AGNs are similarly related with beaming effect. The cosmological expanding effect would play no part in the superluminal motion of radio galaxies, BL Lacertae objects as well as quasars. Meanwhile, we confirm that estimates for apparent velocity β app and Doppler boosting factor δ based on multi-wavelength combination and variability are comparable.

Affiliated with

Also associated with

No associations

Rating

On the Superluminal Motion of Radio-Loud AGNs 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 On the Superluminal Motion of Radio-Loud AGNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Superluminal Motion of Radio-Loud AGNs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-919258