Open AccessXMM–Newton observations of three high‐redshift radio galaxies
Author(s) -
Belsole E.,
Worrall D. M.,
Hardcastle M. J.,
Birkinshaw M.,
Lawrence C. R.
Publication year - 2004
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2004.07983.x
Subject(s) - physics , astrophysics , radio galaxy , redshift , luminosity , astronomy , galaxy , galaxy cluster , active galactic nucleus , x shaped radio galaxy
We present the results of XMM–Newton observations of three powerful high‐redshift radio galaxies 3C 184, 3C 292 and 3C 322. Although none of the sources lies in as rich an X‐ray‐emitting environment as is seen for some powerful radio galaxies at low redshift, the environments provide sufficient pressure to confine the radio lobes. The weak gas emission is particularly interesting for 3C 184, where a gravitational arc is seen, suggesting the presence of a massive cluster. Here, Chandra data complement the XMM–Newton measurements by spatially separating X‐rays from the extended atmosphere, the nucleus and the small‐scale radio source. For 3C 292, the X‐ray‐emitting gas has a temperature of ∼2 keV and a luminosity of 6.5 × 10 43 erg s −1 , characteristic of a poor cluster. In all three cases, structures where the magnetic‐field strength can be estimated through combining measurements of radio synchrotron and inverse‐Compton X‐ray emission are consistent with being in a state of minimum total energy. 3C 184 and 3C 292 (and possibly 3C 322) have a heavily absorbed component of nuclear emission of N H ∼ few times 10 23 cm −2 .