Published April 1991
| Version v1
Journal article
A long-lasting compact group
- 1. Padova, Osservatorio Astronomico, Padua (Italy)
- 2. Osservatorio Astronomico di Brera, Milan (Italy)
- 3. Milano, Universita, Milan (Italy)
- 4. Osservatorio Astronomico di Brera (Italy)
Description
The dynamical evolution of a compact group of four galaxies has been studied using Aarseth's NBODY2 code. An important departure from previous studies is the wider range of masses chosen for the individual galaxies, which are representative of those existing in Hickson's catalog. The first merging occurs after 4.3 billion yr, while the group lasts for as many as nine billion yr before merging into a single remnant. Two other simulations test the dependence of the results on the galaxy models adopted and the general set of initial conditions. Another run, with four identical galaxies and no special initial conditions, is used as a standard of reference. 13 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 371
- Series
- Astrophys. J.
- Journal Page Range
- L15-L18
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22078876
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COMPUTERIZED SIMULATION; GALACTIC EVOLUTION; GALAXY CLUSTERS; GRAVITATIONAL INTERACTIONS; MASS; MATHEMATICAL MODELS; N CODES
- Descriptors DEC
- BASIC INTERACTIONS; COMPUTER CODES; SIMULATION
Optional Information
- Notes
- L15-L18.