X-ray Spectroscopy of BAL and Mini-BAL QSOs

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dc.creatorGallagher, S. C.
dc.creatorBrandt, W. N.
dc.creatorChartas, G.
dc.creatorGarmire, G. P.
dc.date2001-05-18
dc.date.accessioned2026-07-07T01:58:38Z
dc.date.available2026-07-07T01:58:38Z
dc.descriptionBAL QSOs are notoriously faint X-ray sources, presumably due to extreme intrinsic absorption. However, several objects have begun to appear through the obscuration with recent X-ray observations by Chandra and ASCA. Where enough counts are present for X-ray spectroscopy, the signatures of absorption are clear. The evidence is also mounting that the absorbers are more complicated than previous simple models assumed; current absorber models need to be extended to the high-luminosity, high-velocity, and high-ionization regime appropriate for BAL QSOs.
dc.description6 pages, 4 postscript figures, LaTeX, requires newpasp.sty. To appear in the conference proceedings for Mass Outflow in AGN: New Perspectives, ASP Conference Series, eds. D. M. Crenshaw, S. B. Kraemer, and I. M. George
dc.identifierhttps://arxiv.org/abs/astro-ph/0105332
dc.identifierhttp://arxiv.org/abs/astro-ph/0105332
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2790
dc.subjectAstrophysics
dc.titleX-ray Spectroscopy of BAL and Mini-BAL QSOs
dc.typetext

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