Published May 1979
| Version v1
Journal article
The evolution of cluster X-ray sources: subcluster collisions
Description
The evolution of cluster X-ray sources is investigated with a three-dimensional hydrodynamical numerical technique. Particular attention has been paid to the behaviour of intracluster gas during the merger of two subclusters to form a single cluster. Only a small enhancement is found in X-ray luminosity during the merger. The evolution of the X-ray luminosity subsequent to the merger is very similar to that found previously with a one-dimensional code. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 187
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 371-378
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 10471818
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC GASES; COSMIC X-RAY SOURCES; COSMOLOGICAL MODELS; GALACTIC EVOLUTION; GALAXY CLUSTERS; HYDRODYNAMICS; LUMINOSITY; X RADIATION
- Descriptors DEC
- COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; FLUID MECHANICS; FLUIDS; GASES; IONIZING RADIATIONS; MATHEMATICAL MODELS; MECHANICS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS