Published June 1990 | Version v1
Journal article

The Extended Medium Sensitivity Survey distant cluster sample - X-ray cosmological evolution

  • 1. Colorado Univ., Boulder (USA)
  • 2. Mount Wilson and Las Campanas Observatories, Pasadena, CA (USA)
  • 3. Osservatorio Astronomico, Bologna (Italy)
  • 4. Hawaii Univ., Honolulu (USA)
  • 5. CNR, Istituto di Radioastronomia, Bologna (Italy)
  • 6. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)

Description

The X-ray luminosity function of clusters of galaxies is determined at different cosmic epochs using data from the Einstein Observatory Extended Medium Sensitivity Survey. The sample consists of 67 X-ray-selected clusters that have been grouped in three redshift shells. Evolution is detected in the X-ray properties of clusters. The present volume density of high-luminosity clusters is found to be greater than it was in the past. Given the still limited data set, this result should be regarded as preliminary. It can be interpreted as the consequence of either luminosity evolution or modest density evolution. 22 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
356
Series
Astrophys. J.
Journal Page Range
L35-L38
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
21085279
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ASTROPHYSICS; COSMOLOGY; DENSITY; GALACTIC EVOLUTION; GALAXY CLUSTERS; LUMINOSITY; RED SHIFT; X RADIATION
Descriptors DEC
ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS