SUMMARY OF PROPOSAL 62135

DR. PAUL J. GREEN
PGREEN@CFA.HARVARD.EDU

SMITHSONIAN INSTITUTION ASTROPHYSICAL OBSERVATORY
60 GARDEN ST.
CAMBRIDGE
MA/MIDDLESEX USA 02138
Tel: (617)495-7057 Fax: (617)496-7577
Medium: 2GBDAT
Subject: AGN

DEEP CAMPAIGN TO PROBE ONE TYPICAL BROAD ABSORPTION LINE QSO


ABSTRACT

We propose a deep ASCA observation of one representative broad absorption line (BAL) QSO. PG0946+301 has been chosen as the best target for our large collaborative campaign. Deep ASCA spectroscopy will provide the first high quality measurements of the ionizing continuum and total column density of the warm absorbers in BALQSOs. Photoionization modeling of this spectrum, combined with existing HST and ground-based optical spectra, will enable us to characterize the dynamics, ionization, and metallicity of the outflows. Results for this typical BALQSO are immediately generalizeable to BALQSOs as a class. Since BALQSOs are probably normal QSOs viewed along a sightline passing through a BAL outflow, we expect to provide a unique probe of conditions near the nucleus of most QSOs.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
SMITA MATHURSAOUSA
CHIKO OTANIRIKENJAPAN
JOSEPH SHIELDSOHIO UUSA
FRED HAMANNUCSDUSA
KIRK KORISTAU. KENTUCKYUSA
NAHUM ARAVCALTECHUSA
MICHAEL BROTHERTONLLNLUSA
MARTIJN DEKOOLU. COLORADOUSA
MARTIN ELVISSAOUSA
BRADLEY PETERSONOHIO STATEUSA

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)PG0946+301
2
147.4212 29.9218 100 ksN
N
P
0.02890
1

TARGET 1

SOURCE IS PROBABLY HIGHLY ABSORBED.