Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-29T09:46:04.323Z Has data issue: false hasContentIssue false
  • English
  • Français

Superwind and Chain Galaxy Formation at High Redshift

Published online by Cambridge University Press:  26 May 2016

Yasuhiro Shioya  and
Yoshiaki Taniguchi
Yasuhiro Shioya
Affiliation:
Astronomical Institute, Tohoku University, Sendai, 980-8578, Japan
Yoshiaki Taniguchi
Affiliation:
Astronomical Institute, Tohoku University, Sendai, 980-8578, Japan

Abstract

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.

We propose a possible new model for the formation of chain galaxies at high redshift.

Type
Part 4. Recycling
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 504 - 505
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Cowie, L. L., Hu, E. M., & Songaila, A. 1995, AJ, 110, 1576.CrossRefGoogle Scholar
Taniguchi, Y. & Shioya, Y. 2001, ApJ, 547, 146.Google Scholar
van den Bergh, S., et al. 1996, AJ, 112, 359.CrossRefGoogle Scholar