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.