SUMMARY OF PROPOSAL 72093

DR. JOHN S. ARABADJIS
JSA@ASTRO.LSA.UMICH.EDU

UNIVERSITY OF MICHIGAN
500 CHURCH STREET
ANN ARBOR
MICHIGAN USA 48109-1090
Tel: (734) 764-3412 Fax: (734) 763-6317
Medium: CD ROM
Subject: AGN

THE MASS AND DISTRIBUTION OF MOLECULAR GAS IN THE GALAXY


ABSTRACT

Molecular absorption line studies and X-ray absorption observations toward extragalactic sight lines indicate that molecular gas is as abundant as neutral atomic gas in the Solar vicinity. At larger Galactic radii, H2 exceeds HI in some locations, and if this is generally true, it implies a dramatic revision in the picture of neutral gas in disk galaxies. To determine if H2 dominates the ISM at large radii, we propose to measure the X-ray absorption column toward AGNs projected behind the outer part of the Galactic disk, which is expected to be about 1E22/cm2. The H2 column is the difference between the X-ray absorption column and the observed HI 21 cm column.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
JOEL BREGMANUNIV. OF MICHIGANUSA

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)1RXSJ024457.8+622810
C
41.2408 62.4696
20 ks
N
N
P
0.98590
1
2)1RXSJ003552.8+595006
C
8.9700 59.8350
20 ks
N
N
P
0.88260
1
3)1RXSJ013748.0+581422
C
24.4500 58.2396
20 ks
N
N
P
0.69980
1