Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-06-13
2011ScChG..54..183C
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
4 pages, 1 figures, Science China: G accepted
Scientific paper
10.1007/s11433-010-4153-4
PG 1407+265 is a radio quiet quasar but has a relativistic jet. In this report, we show some peculiar properties of its optical and X-ray emissions, which indicate their possible non-thermal origins produced from jet. We use a simple synchrotron + synchrotron self Compton (SSC) model to fit the emissions with different ratios of energy densities between magnetic field and electrons (\eta=UB/Ue), which predict different {\gamma}-ray luminosity. The First LAT AGN Catalog (1LAC) did not include PG 1407+265, which indicates an upper limit of {\gamma}-ray luminosity. This upper limit constrains the ratio unreasonable large (\eta>10^4-10^5). This inversely indicates that the optical and X-ray emissions may be not produced from the beaming jet. We discuss the physical implications of these results.
Bai Jin-Ming
Chen Liang
No associations
LandOfFree
A puzzle of radio-quiet quasar PG 1407+265: are optical and X-ray emissions produced from relativistic jet? 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 A puzzle of radio-quiet quasar PG 1407+265: are optical and X-ray emissions produced from relativistic jet?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A puzzle of radio-quiet quasar PG 1407+265: are optical and X-ray emissions produced from relativistic jet? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-625586