… As described in de Blok et al. (2008), the resulting rotation curve resembles that of a galaxy
… In this paper, we use the Hermite h 3 rotation curve derived in de Blok et al. (2008) for the …

… In general, the minimum disk assumption is a good description for dwarf galaxies and LSB
galaxies (de Blok & Bosma 2002), and we therefore also apply this assumption to IC 2574 …

… profiles in galaxy halos are too steep; cf., de Blok et al. 2001) is another manifestation of the
(… We adopt luminosities and distances as given in Walter et al. (2008), and where necessary …

We make a direct comparison of the derived dark matter (DM) distributions between
hydrodynamical simulations of dwarf galaxies assuming a ΛCDM cosmology and the observed …

We present several results from our analysis of dwarf irregular galaxies culled from The HI
Nearby Galaxy Survey (THINGS). We analyse the rotation curves of two galaxies based on “…

We present high-resolution (∼ 6) rotation curves of IC2574 and NGC 2366 from ‘The H i
Nearby Galaxy Survey’(THINGS)[1] as shown in the top panels of Fig. 1. In order to minimize the …

MHONGOOSE is a deep survey of the neutral hydrogen distribution in a representative sample
of 30 nearby disk and dwarf galaxies with HI masses from 10^6 to ~10^{11} M_sun, and …

Observed H i accretion around nearby galaxies can only account for a fraction of the gas
supply needed to sustain the currently observed star formation rates. It is possible that …

… In this paper, we decompose all the line profiles of the ATCA H i data cube of NGC 6822 (de
Blok & Walter 2000) with an optimal number of Gaussian components using baygaud, and …

… We adopt M HI from Walter et al. (2008), scaling by 1.36 to account for helium. The stellar …
a Kroupa IMF (NGC 2903 comes from de Blok et al. 2008). de Blok et al. (2008) investigate …