Bibcode
DOI
Wang, J. X.; Wang, T. G.; Tozzi, P.; Giacconi, R.; Hasinger, G.; Kewley, L.; Mainieri, V.; Nonino, M.; Norman, C.; Streblyanska, A.; Szokoly, G.; Yaqoob, T.; Zirm, A.
Bibliographical reference
The Astrophysical Journal, Volume 631, Issue 1, pp. L33-L36.
Advertised on:
9
2005
Journal
Citations
8
Refereed citations
8
Description
In this Letter we report the detection of a strong and extremely
blueshifted X-ray absorption feature in the 1 Ms Chandra spectrum of
CXOCDFS J033260.0-274748, a quasar at z=2.579 with
L2-10keV~4×1044 ergs s-1. The
broad absorption feature at ~6.3 keV in the observed frame can be fitted
either as an absorption edge at 20.9 keV or as a broad absorption line
at 22.2 keV rest frame. The absorber has to be extremely ionized with an
ionization parameter ξ~104, and a high column density,
NH>5×1023 cm-2. We reject the
possibility of a statistical or instrumental artifact. The most likely
interpretation is an extremely blueshifted broad absorption line or
absorption edge, due to H or He-like iron in a relativistic jetlike
outflow with bulk velocity of ~0.7c-0.8c. Similar relativistic outflows
have been reported in the X-ray spectra of several other AGNs in the
past few years.