Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-12T20:03:45.974Z Has data issue: false hasContentIssue false

Simulations of Compact Groups of Galaxies with Halos

Published online by Cambridge University Press:  04 August 2017

T. Ishizawa*
Affiliation:
Department of Astronomy, University of Kyoto

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Self-consistent simulations of seven groups are performed from the maximum expansion to the present using Aarseth's N-body code. An initial galaxy consists of 100 stars. Its mass, half-mass radius, and central velocity dispersion are 1, 0.41, and 0.96. Units of mass, length, velocity, and time are 1.4×101 2M, 100 kpc, 245 kms−1 and 4.0×108y. Table 1 gives the elapsed time from the Big Bang to the formation of a multiple merger tm+Tc*/2. For H0=80 kms−1Mpc−1, the Hubble time H0−1=30.6 in our units. Dense groups except B form multiple mergers in a Hubble time.

Type
Research Article
Copyright
Copyright © Reidel 1987 

References

Geller, M. J. and Huchra, J.P. 1983, Astrophys. J. Suppl. 52, 61.CrossRefGoogle Scholar