THE CIRCULAR VELOCITY FUNCTION OF GROUP GALAXIES
A robust prediction of ACDM cosmology is the halo circular velocity function (CVF), a dynamical cousin of the halo mass function. The correspondence between theoretical and observed CVFs is uncertain, however: cluster galaxies are reported to exhibit a power-law CVF consistent with N-body simulation...
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Veröffentlicht in: | The Astrophysical journal 2014-09, Vol.793 (1), p.1-15 |
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Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | A robust prediction of ACDM cosmology is the halo circular velocity function (CVF), a dynamical cousin of the halo mass function. The correspondence between theoretical and observed CVFs is uncertain, however: cluster galaxies are reported to exhibit a power-law CVF consistent with N-body simulations, but that of the field is distinctly Schechter-like, flattened compared to ACDM expectations at circular velocities [upsilon] sub(c) [ |
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ISSN: | 1538-4357 0004-637X 1538-4357 |
DOI: | 10.1088/0004-637X/793/1/49 |