Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-04-30
Mon.Not.Roy.Astron.Soc. 342 (2003) L53
Astronomy and Astrophysics
Astrophysics
5 pages, 3 figures, accepted for publication in MNRAS
Scientific paper
10.1046/j.1365-8711.2003.06736.x
We present XMM-Newton observations and spectral fitting of two highly redshift, [OIII]-luminous, narrow-line radio galaxies, B3 0731+438 and 3C 257. Their X-ray continua are well fitted by a partial covering model with intrinsically unabsorbed and absorbed powerlaw components. The spectral models indicate that both objects harbour highly obscured nuclei, with N_H ~ 0.5 - 2 x 10^23 cm^-2. Correcting for this absorption we find large intrinsic luminosities in the range L_X ~ 0.2 - 1 x 10^45 erg/s. Thus, both sources are type-2 quasars.
Derry P. M.
Imanishi Masatoshi
O'Brien Thomas P.
Reeves James N.
Ueno Satoru
No associations
LandOfFree
Detection of type-2 quasars in the radio galaxies B3 0731+438 and 3C 257 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 Detection of type-2 quasars in the radio galaxies B3 0731+438 and 3C 257, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of type-2 quasars in the radio galaxies B3 0731+438 and 3C 257 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-31185