Soft Cores in Late-Type Dwarf and LSB Galaxies from HαObservations

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We present high spatial resolution Hαrotation curves of late-type dwarf and LSB galaxies. From our analysis we find good agreement between our Hαdata and the HI observations taken from the literature, concluding that the HI rotation curves for these galaxies suffer very little from beam smearing. A preliminary analysis of our data rules out the CDM model in the inner regions of these galaxies.
Contribution to "Tracing Cosmic Evolution with Galaxy Clusters" (Sesto 2001), ASP Conference Series

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/3097

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0107424
 http://arxiv.org/abs/astro-ph/0107424

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arXiv