All Tables

Table 1: Basic properties of the dwarf irregular galaxy ESO 364-G029. The left and middle columns list the different quantities and their values; the right column lists corresponding references - (1) NED; (2) HyperLEDA; (3) This paper; (4) Karachentsev et al. (2004).
Table 2: Parameters of the ATCA H I observations. Observations were obtained in four different configurations, and combined (see Sect. 3) for analysis.
Table 3: Properties of the four datacubes used in our analysis. For the analysis of the detailed morphology of ESO 364-G029 we use the long-baseline datacubes NL and UL, which have a high spatial resolution. For the derivation of the global structure of ESO 364-G029 we use the datacubes NH and UH, which contain only the short baseline observations. The latter datasets are therefore deeper than the former, but have lower spatial resolutions.
Table 4: Basic properties of galaxies near ESO 364-G029. This table lists all galaxies with a projected distance differing by less than $5\hbox {$^\circ $ }$ and a redshift differing by less than 500 km s^-1 from ESO 364-G029. Only galaxies with a known redshift are included. From left to right, the columns list the galaxy name, spectral type, total apparent B magnitude and the angular separation, projected separation (assuming a distance of 10.8 Mpc), and relative radial velocity from ESO 364-G029.