Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 360, Issue 4, Pages 1201-1230Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2005.09125.x
Keywords
methods : observational; techniques : radial velocities; galaxies : fundamental parameters; galaxies : kinematics and dynamics; galaxies : spiral
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We present the H alpha gas kinematics of 21 representative barred spiral galaxies belonging to the BH alpha BAR sample. The galaxies were observed with FaNTOmM, a Fabry-Perot integral-field spectrometer, on three different telescopes. The three-dimensional data cubes were processed through a robust pipeline with the aim of providing the most homogeneous and accurate data set possible useful for further analysis. The data cubes were spatially binned to a constant signal-to-noise ratio, typically around 7. Maps of the monochromatic H alpha emission line and of the velocity field were generated and the kinematical parameters were derived for the whole sample using tilted-ring models. The photometrical and kinematical parameters (position angle of the major axis, inclination, systemic velocity and kinematical centre) are in relative good agreement, except perhaps for the later-type spirals.
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