Publication | Open Access
HI observations of nearby galaxies V. Narrow (HI) line galaxies
53
Citations
8
References
2003
Year
Galaxy FormationPhotometryEngineeringAstrostatisticsHi ProfilesAstrodynamicsAstronomical Image AnalysisLarge Scale StructureObserved Line WidthHigh Velocity ResolutionHi Observations
In this paper we present new HI observations with high velocity resolution for 104 nearby narrow-line galaxies with half power line widths smaller than 50 km s-1 most of which are well approximated by a Gaussian. The FWHM line width of 30 of these integrated HI profiles is less than 25 km s-1. We present global parameters of these nearby galaxies and discuss the size dependence, the luminosity dependence, and the dependence of these parameters with the observed line width. Our sample essentially is a subsample of the Local Volume (i.e. galaxies within 10 Mpc) with declinations ≥-30° and only a few galaxies at greater distances. It is described by the following median values of global physical parameters: total absolute blue magnitude ; linear diameter kpc (this corresponds to the de Vaucouleurs diameter D25); half power line width km s-1; total HI mass ; distance Mpc; HI mass-to-luminosity ratio ; total mass-to luminosity ratio .
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