Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

SUZAKU OBSERVATIONS OF NEAR-RELATIVISTIC OUTFLOWS IN THE BAL QUASAR APM 08279+5255

Journal Article · · Astrophysical Journal
We present results from three Suzaku observations of the z = 3.91 gravitationally lensed broad absorption line quasar APM 08279+5255. We detect strong and broad absorption at rest-frame energies of {approx}<2 keV (low energy) and 7-12 keV (high energy). The detection of these features confirms the results of previous long-exposure (80-90 ks) Chandra and XMM-Newton observations. The low- and high-energy absorption is detected in both the back-illuminated (BI) and front-illuminated (FI) Suzaku X-ray Imaging Spectrometer spectra (with an F-test significance of {approx}>99%). We interpret the low-energy absorption as arising from a low-ionization absorber with log N {sub H} {approx} 23 and the high-energy absorption as due to lines arising from highly ionized (2.75 {approx}< log{xi} {approx}< 4.0, where {xi} is the ionization parameter) iron in a near-relativistic outflowing wind. Assuming this interpretation we find that the velocities in the outflow range between 0.1c and 0.6c. We constrain the angle between the outflow direction of the X-ray absorber and our line of sight to be {approx}<36 deg. We also detect likely variability of the absorption lines (at the {approx}>99.9% and {approx}>98% significance levels in the FI and BI spectra, respectively) with a rest-frame timescale of {approx}1 month. Assuming that the detected high-energy absorption features arise from Fe XXV, we estimate that the fraction of the total bolometric energy injected over the quasar's lifetime into the intergalactic medium in the form of kinetic energy to be {approx}>10%.
OSTI ID:
21300598
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 697; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

A STUDY OF THE X-RAYED OUTFLOW OF APM 08279+5255 THROUGH PHOTOIONIZATION CODES
Journal Article · Sat Aug 20 00:00:00 EDT 2011 · Astrophysical Journal · OSTI ID:21579934

CONFIRMATION OF AND VARIABLE ENERGY INJECTION BY A NEAR-RELATIVISTIC OUTFLOW IN APM 08279+5255
Journal Article · Thu Nov 19 23:00:00 EST 2009 · Astrophysical Journal · OSTI ID:21378150

AKARI NEAR- AND MID-INFRARED SPECTROSCOPY OF APM 08279+5255 AT z = 3.91
Journal Article · Wed May 20 00:00:00 EDT 2009 · Astrophysical Journal · OSTI ID:21300588