Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-29T18:33:08.806Z Has data issue: false hasContentIssue false
  • English
  • Français

HI Observations of the Interacting Galaxies - VV 371 and VV 329

Published online by Cambridge University Press:  04 August 2017

Edwin J. Grayzeck
Edwin J. Grayzeck*
Affiliation:
University of Nevada Las Vegas

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.

Recent evidence for the tidal interaction among neighboring galaxies in the form of HI bridges and streamers has been accumulated by Haynes (1981). The successful application of computer simulations to model these encounters has largely been restricted to the nearby systems such as the Milky Way. In this paper, I will report on preliminary observations of the HI distributions associated with two interacting systems - VV 371 and VV 329.

Type
I. Kinematics of Gas and the Underlying Mass Distribution
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 97 - 98
Copyright
Copyright © Reidel 1983 

References

Haynes, M. 1981, Astron. J., 86, 1126.Google Scholar
Hewitt, J., Haynes, M., and Giovanelli, R. 1982, preprint.Google Scholar
Mirabel, F. 1982, preprint.Google Scholar
Vorontsov-Velyaminov, B.A. 1977, Astron. Astrophys. Suppl., 28, 1.Google Scholar