Abstract
Aims. We present new 2D high resolution Fabry–Perot spectroscopic observations of 152 star-forming galaxies that are part of the Herschel Reference Survey (HRS), which is a complete K-band selected, volume-limited sample of nearby galaxies that spans a wide range of stellar mass and morphological types. Methods. By using improved data reduction techniques, that provide adaptive binning based on Voronoi tessellation, and using large field-of-view observations, we derived high spectral resolution (R > 10 000) Hα datacubes from which we computed Hα maps and radial 2D velocity fields that are based on several of thousand independent measurements. A robust method based on such fields allowed us to accurately compute rotation curves and kinematical parameters, for which uncertainties are calculated using a method based on the power spectrum of the residual velocity fields. Results. We checked the consistency of the rotation curves by comparing our maximum rotational velocities to those derived from H I data, and by computing the i-band, NIR, stellar, and baryonic Tully-Fisher relations. We used this set of kinematical data combined with those available at other frequencies to study, for the first time, the relation between the dynamical and the total baryonic mass (stars, atomic and molecular gas, metals, and dust) and to derive the baryonic and dynamical main sequence on a representative sample of the local universe.
Highlights
One of the main processes regulating galaxy evolution is star formation
The Herschel Reference Survey (HRS) is a K-band-selected, volume-limited (15 < D < 25 Mpc) complete sample of 323 galaxies spanning a wide range in morphological type and stellar mass (108 < Mstar < 1011 M )
Rotation curves are computed from the velocity fields following the method described in Epinat et al (2008b), which is a synthesis adapted to Hα data between the angular sector method, tiltedring models and the fitting method used by Barnes & Sellwood (2003)
Summary
One of the main processes regulating galaxy evolution is star formation. The gas located along the disk of spiral galaxies collapses inside molecular clouds to form stars following the Kennicutt–Schmidt law (Schmidt 1959; Kennicutt 1989). The Herschel Reference Survey (HRS, Boselli et al 2010) is a complete sample of 323 nearby galaxies that aims to study the relationship between the star formation process and the different components of the ISM This sample has been observed at all frequencies in order to provide the community with the largest possible set of homogeneous data. This paper presents new Fabry–Perot data for 152 HRS starforming galaxies gathered during nine observing runs at the Observatoire de Haute Provence (OHP) These data are used to derive the kinematical properties of the ionized gas at high spatial and spectral resolution. By combining this new set of data with other Fabry–Perot data available in the literature, we study the relationship between the dynamical and the baryonic mass. Consistent with our previous works, all of the Fabry–Perot data are made available on the HRS dedicated database HeDAM1 and on the Fabry–Perot database
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