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J/A+A/370/765 HI synthesis observations in UMa cluster (Verheijen+, 2001)
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Beginning of ReadMe :J/A+A/370/765 HI synthesis observations in UMa cluster (Verheijen+, 2001)
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The Ursa Major cluster of galaxies. IV. HI synthesis observations.
Verheijen M.A.W., Sancisi R.
<Astron. Astrophys. 370, 765 (2001)>
=2001A&A...370..765V
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ADC_Keywords: Clusters, galaxy ; H I data ; Galaxies, rotation ; Photometry
Keywords: galaxies: fundamental parameters - galaxies: kinematics and dynamics -
galaxies: spiral - galaxies: structure
Abstract:
In this data paper we present the results of an extensive 21 cm-line
synthesis imaging survey of 43 spiral galaxies in the nearby Ursa
Major cluster using the Westerbork Synthesis Radio Telescope. Detailed
kinematic information in the form of position-velocity diagrams and
rotation curves is presented in an atlas together with HI channel
maps, 21 cm continuum maps, global HI profiles, radial HI surface
density profiles, integrated HI column density maps, and HI velocity
fields. The relation between the corrected global HI linewidth and the
rotational velocities Vmax and Vflat as derived from the rotation
curves is investigated. Inclination angles obtained from the optical
axis ratios are compared to those derived from the inclined HI disks
and the HI velocity fields. The galaxies were not selected on the
basis of their HI content but solely on the basis of their cluster
membership and inclination which should be suitable for a kinematic
analysis. The observed galaxies provide a well-defined, volume limited
and equidistant sample, useful to investigate in detail the
statistical properties of the Tully-Fisher relation and the dark
matter halos around them.