Dramatic X-ray Spectral Variability of the Broad Absorption Line Quasar PG2112+059

With a 1999 ASCA observation, PG2112+059 became notable as the first Broad Absorption Line (BAL) quasar found to exhibit a typical radio-quiet quasar X-ray continuum underlying a large amount of intrinsic absorption. We present a recent Chandra ACIS-S3 observation of PG2112+059 that demonstrates remarkable spectral and luminosity variability since that time. In addition to a decrease in the continuum normalization by a factor of ~3.5, the absorption column density has apparently increased substantially, and a strong feature in the Fe K alpha region has appeared. Concurrent HST STIS data compared with archival HST data from earlier epochs show evidence for variability of the continuum (up to a factor of ~1.7 in the ultraviolet), and in some absorption features of the CIV 1549 BAL since 1992; however, the OVI BAL structure is consistent with a 1995 observation. We also present evidence for Ly beta--OVI 1037.62 and Ly alpha--NV 1242.80 line-locked absorption systems, supporting the assumption that ultraviolet line pressure is driving the BAL outflow. Whereas ultraviolet BALs typically exhibit only modest equivalent-width variability over timescales of years, the dramatic X-ray variability of PG2112+059 suggests that X-ray spectral variability studies of BAL quasars have great potential for probing the physics of quasar winds.