arXiv · 1608.01677
The Califa and Hipass velocity function for all morphological galaxy types
Abstract
The velocity function is a fundamental observable statistic of the galaxy population, similarly impor- tant as the luminosity function, but much more difficult to measure. In this work we present the first directly measured circular velocity function that is representative between 60 < v_circ < 320 km/s for galaxies of all morphological types at a given rotation velocity. For the low mass galaxy population (60 < v_circ < 170 km/s), we use the HIPASS velocity function. For the massive galaxy population (170 < v_circ < 320 km/s), we use stellar circular velocities from the Calar Alto Legacy Integral Field Area Survey (CALIFA). In earlier work we obtained the measurements of circular velocity at the 80% light radius for 226 galaxies and demonstrated that the CALIFA sample can produce volume- corrected galaxy distribution functions. The CALIFA velocity function includes homogeneous velocity measurements of both late and early-type rotation-supported galaxies and has the crucial advantage of not missing gas-poor massive ellipticals that HI surveys are blind to. We show that both velocity functions can be combined in a seamless manner, as their ranges of validity overlap. The resulting observed velocity function is compared to velocity functions derived from cosmological simulations of the z = 0 galaxy population. We find that dark matter-only simulations show a strong mismatch with the observed VF. Hydrodynamic simulations fare better, but still do not fully reproduce observations.
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S. Bekeraitė, C. J. Walcher, L. Wisotzki, D. J. Croton, J. Falcón-Barroso, M. Lyubenova, D. Obreschkow, S. F. Sánchez, K. Spekkens, P. Torrey, G. van de Ven, M. A. Zwaan, Y. Ascasibar, J. Bland-Hawthorn, R. González-Delgado, B. Husemann, R. A. Marino, M. Vogelsberger, B. Ziegler, the CALIFA collaboration. 2016-08-04. The Califa and Hipass velocity function for all morphological galaxy types. https://doi.org/10.3847/2041-8205%2F827%2F2%2Fl36
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