SUMMARY OF PROPOSAL 72188

DONALD J HORNER
HORNER@MILKYWAY.GSFC.NASA.GOV

GODDARD SPACE FLIGHT CENTER

GREENBELT
MD USA 20771
Tel: 301-286-1132 Fax: 301-286-1684
Medium: CD ROM
Subject: CLUSTERS OF GALAXIES AND SUPERCLUSTERS

THE MASS--TEMPERATURE RELATIONSHIP OF GALAXY CLUSTERS


ABSTRACT

Theoretical arguments and simulations suggest that the total mass of a galaxy cluster is tightly correlated to its x-ray temperature and that the lower end of the M-T relationship is sensitive to non-gravitational effects, such as energy injection by galactic winds. We have investigated the M-T relationship for a variety of mass estimation techniques. We propose ASCA observations of a sample of six low mass clusters to obtain accurate x-ray temperatures. This will nearly the double the number of clusters with accurate virial masses and ASCA temperatures in the region 2--3 keV and will allow a determination of the scaling of viral mass and temperature over the full range of rich cluster masses.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
RICHARD MUSHOTZKYLHEA/GSFCUSA
CALEB SCHARFSTSCIUSA

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)ABELL 1142
C
165.2292 10.5478
20 ks
N
N
P
1.10000
1
2)ABELL 2589
B
351.0021 16.8247
20 ks
N
N
P
0.80000
1
3)ABELL 2593
C
351.1292 14.6414
30 ks
N
N
P
0.60000
1