Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-26T22:18:11.380Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular hydrogen as dark mass in dwarf galaxies

Published online by Cambridge University Press:  26 May 2016

P. R. Williams ,
C. Marzok ,
S. Myers  and
A. H. Nelson
P. R. Williams
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, PR China
C. Marzok
Affiliation:
Department of Physics and Astronomy, Cardiff University, Cardiff CF2 3YB, Wales, UK
S. Myers
Affiliation:
Department of Physics and Astronomy, Cardiff University, Cardiff CF2 3YB, Wales, UK
A. H. Nelson
Affiliation:
Department of Physics and Astronomy, Cardiff University, Cardiff CF2 3YB, Wales, UK

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 report here an example of a series of computer simulations of the formation of disk galaxies, including a standard cold dark matter component, gas, and star formation, which result in objects which closely resemble observed giant galaxies, with a population of long-lived dwarf satellites which contain little or no non–baryonic dark matter.

Type
Part 7: Baryonic Dark Matter
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 251 - 252
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Braine, J., et al., A&A, 2001, 378, 51.Google Scholar
Elmegreen, B. G., Hunter, D. A., 2000, ApJ, 540, 814.Google Scholar
Lisenfeld, U., et al., 2002, A&A, 382, 860.Google Scholar
Papadopoulos, P. P., et al., 2002, ApJ, 579, 270.Google Scholar
Valentijn, E. A., van der Werf, P. P., 1999, ApJ, 522, L29.Google Scholar
Williams, P. R., Nelson, A. H., 2001, A&A, 374, 839.Google Scholar