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Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation

Published online by Cambridge University Press:  21 October 2010

M. Bureau ,
M. J. Williams  and
M. Cappellari
M. Bureau
Affiliation:
University of Oxford, UK
M. J. Williams
Affiliation:
University of Oxford, UK
M. Cappellari
Affiliation:
University of Oxford, UK
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We provide observational constraints on disk galaxy evolution for a sample of 28 local edge-on early-type (S0–Sb) disk galaxies. We do this in two ways: (i) we use simple dynamical modelling techniques to constrain their stellar and dark matter content (Williams et al. 2009) and (ii) we compare the zero points of the Tully-Fisher relations (TFRs; Tully & Fisher 1977) of the spirals and S0s.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 82
Copyright
Copyright © International Astronomical Union 2010

References

Bedregal, A. G., Aragón-Salamanca, A., & Merrifield, M. R., 2006, MNRAS, 373, 1125CrossRefGoogle Scholar
Cappellari, M., 2008, MNRAS, 390, 71CrossRefGoogle Scholar
Tully, R. B. & Fisher, J. R., 1977, A&A, 54, 661Google Scholar
Williams, M. J., Bureau, M., & Cappellari, M., 2009, MNRAS, acceptedGoogle Scholar