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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

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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

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