Hostname: page-component-669899f699-7xsfk Total loading time: 0 Render date: 2025-04-27T08:43:15.616Z Has data issue: false hasContentIssue false
  • English
  • Français

Inner Halo Shapes of Dwarf Galaxies: Resolving the Cusp/Core Problem

Published online by Cambridge University Press:  26 May 2016

Kristine Spekkens  and
Riccardo Giovanelli
Kristine Spekkens
Affiliation:
Cornell University, Space Sciences Building, Ithaca, NY 14853, USA
Riccardo Giovanelli
Affiliation:
Cornell University, Space Sciences Building, Ithaca, NY 14853, USA

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 derive inner dark matter halo density profile slopes for a sample of 200 dwarf galaxies by inverting rotation curves obtained from high-quality, long-slit optical spectra. Using simulations to assess the impact of long-slit observing and data processing errors on our measurements, we conclude that our observations are consistent with the cuspy halos predicted by the CDM paradigm.

Type
Part 11: Dwarf Galaxies
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 371 - 372
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Catinella, B. C., Haynes, M. P., & Giovanelli, R. 2003, in preparation.Google Scholar
de Blok, W. J. G., Bosma, A., & McGaugh, S. 2003, MNRAS, 340, 657 (dBBM).CrossRefGoogle Scholar
Navarro, J. F., Frenk, C. S., & White, S. D. M. 1996, ApJ, 462, 563.Google Scholar
Swaters, R. A., Madore, B. F., van den Bosch, F. C., & Balcells, M. 2003, ApJ, 583, 732 (SMBB).CrossRefGoogle Scholar