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The Westerbork HI survey of spiral and irregular galaxies

2002; EDP Sciences; Volume: 390; Issue: 3 Linguagem: Inglês

10.1051/0004-6361

1432-0746

R. A. Swaters, T. S. van Albada, J. M. van der Hulst, R. Sancisi,

Astrophysics and Star Formation Studies

Neutral hydrogen observations with the Westerbork Synthesis Radio Telescope are presented for a sample of 73 late-type dwarf galaxies. These observations are part of the WHISP project (Westerbork Survey of Spiral and Irregular Galaxies). Here we present maps, velocity fields, global profiles and radial surface density profiles of , as well as masses, radii and line widths. For the late-type galaxies in our sample, we find that the ratio of extent to optical diameter, defined as 6.4 disk scale lengths, is on average 1.8 ± 0.8, similar to that seen in spiral galaxies. Most of the dwarf galaxies in this sample are rich in with a typical of 1.5. The relative content increases towards fainter absolute magnitudes and towards fainter surface brightnesses. Dwarf galaxies with lower average column densities also have lower average optical surface brightnesses. We find that lopsidedness is as common among dwarf galaxies as it is in spiral galaxies. About half of the dwarf galaxies in our sample have asymmetric global profiles, a third has a lopsided distribution, and about half shows signs of kinematic lopsidedness.