Probing broad absorption line quasar outflows: X-ray insights

S. C. Gallagher, W. N. Brandt, G. Chartas, G. P. Garmire, R. M. Sambruna

Research output: Contribution to journalArticle

3 Scopus citations

Abstract

Energetic outflows appear to occur in conjunction with active mass accretion onto supermassive black holes. These outflows are most readily observed in the ∼10% of quasars with broad absorption lines, where the observer's line of sight passes through the wind. Until fairly recently, the paucity of X-ray data from these objects was notable, but now sensitive hard-band missions such as Chandra and XMM-Newton are routinely detecting broad absorption line quasars. The X-ray regime offers qualitatively new information for the understanding of these objects, and these new results must be taken into account in theoretical modeling of quasar winds.

Original languageEnglish (US)
Pages (from-to)2594-2598
Number of pages5
JournalAdvances in Space Research
Volume34
Issue number12 SPEC.ISS.
DOIs
StatePublished - Jan 1 2004

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

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    Gallagher, S. C., Brandt, W. N., Chartas, G., Garmire, G. P., & Sambruna, R. M. (2004). Probing broad absorption line quasar outflows: X-ray insights. Advances in Space Research, 34(12 SPEC.ISS.), 2594-2598. https://doi.org/10.1016/j.asr.2003.02.087