Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...476l..11l&link_type=abstract
Astrophysical Journal Letters v.476, p.L11
Astronomy and Astrophysics
Astronomy
15
Galaxies: Bl Lacertae Objects: General, Gamma Rays: Observations
Scientific paper
In the course of the Compton Gamma Ray Observatory mission, the EGRET telescope has detected 14 BL Lacertae objects in high-energy gamma rays through Phase 4. According to the BL Lac sample in Ciliegi, Bassani, & Caroli, two of these 14 sources are X-ray selected (XBL) and 10 are radio-selected (RBL); two are not listed in this sample. An examination of the radio fluxes and the X-ray fluxes for the BL Lac objects detected by EGRET reveals that it seems a strong radio flux must be present if high-energy gamma rays are to be detected in a BL Lac object, while detection is independent of the X-ray flux of the source. This result is in agreement with the picture of the coaligned radio jet and X-ray jet model of the broadband properties of BL Lac objects. For the BL Lac objects listed in Ciliegi et al. that are not detected by EGRET, co-adding of the EGRET data for the undetected RBLs in such a way that the source positions coincide with each other yields a flux excess at a 3.5 sigma level, but similar co-adding of the EGRET data for the undetected XBLs yields no flux excess.
Bertsch David L.
Dingus Brenda Lynn
Esposito Joseph A.
Fichtel Carl E.
Hartman Robert C.
No associations
LandOfFree
Comparison of X-Ray-- and Radio-selected BL Lacertae Objects in High-Energy Gamma-Ray Observations 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 Comparison of X-Ray-- and Radio-selected BL Lacertae Objects in High-Energy Gamma-Ray Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of X-Ray-- and Radio-selected BL Lacertae Objects in High-Energy Gamma-Ray Observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1775628