SUMMARY OF SEQUENCE NUMBER 700137

SUMMARY OF SEQUENCE NUMBER 700137

Title: RECONCILING UV AND X-RAY OBSERVATIONS OF BALQSO WINDS

Observer: HAMANN

Subject Category: Active Galaxies and Quasars

Seq: 700137 ObsId: 00832

Long-term Plan bin: no LTS bin

ABSTRACT

Recent X-ray observations of BALQSOs indicate absorbing columns that are 2 or more orders of magnitude larger than previous estimates from the UV absorption lines. This huge discrepancy must be resolved if we are to understand even the most basic properties of BAL winds (eg. their mass, location, acceleration, ionization, etc.). I recently used high-quality HST spectra of the bright (V = 15.8), low redshift (z_abs = 0.87) BALQSO PG 1254+047 to derive much larger column densities from the BALs, invoking new evidence that the lines are more optically thick than they appear. I now propose AXAF/ACIS-S observations to 1) test my BAL analysis and 2) place unprecedented constraints on the wind parameters and on the relationship between the UV and X-ray absorbers.

TARGET SUMMARY

TARGET NAME RADEC TIME SI GRAT TYPE TC ROLL PRE PHASE MULTI PRI
PG 1254+047
194.250417
4.459500
40.00000
ACIS-S
NONE
GO
no
no
no
no
no
5

IMAGES

(NOTE: RASS images currently only available for targets LTS scheduled on or after Apr-09-2000)

Roll/Visibility

PARAMETERS

Obscat Parameters