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).
Quantity Value R.
Morphological type IB(s)m 1
Right ascension (J2000) $\alpha=06^{\rm h}05^{\rm m}45\hbox{$.\!\!^{\rm s}$ }2$ 1
Declination (J2000) $\delta=-33\hbox{$^\circ$ }04\hbox{$^\prime$ }51\hbox{$^{\prime\prime}$ }$ 1
Galactic longitude $l=239\hbox{$.\!\!^\circ$ }47$ 1
Galactic latitude $b=-23\hbox{$.\!\!^\circ$ }36$ 1
Heliocentric radial velocity $V_\odot=786 \pm 11$ km s-1 2
    (from H I measurements) $V_\odot=784 \pm 2$ km s-1 3
Scale length (B) $h_B = 50\hbox{$^{\prime\prime}$ }\pm 5\hbox{$^{\prime\prime}$ }$ 3
Radius (25 B mag  ${\rm arcsec}^{-2}$) $R_{25}=1\hbox{$.\mkern-4mu^\prime$ }29 \pm 0\hbox{$.\mkern-4mu^\prime$ }09$ 2
  $R_{25}=1\hbox{$.\mkern-4mu^\prime$ }27 \pm 0\hbox{$.\mkern-4mu^\prime$ }03$ 3
Radius (26.5 B mag  ${\rm arcsec}^{-2}$) $R_{\rm Ho}=2\hbox{$.\mkern-4mu^\prime$ }30 \pm 0\hbox{$.\mkern-4mu^\prime$ }08$ 3
Inclination $i=70\hbox{$.\!\!^\circ$ }5$ 2
Axial ratio (25 B mag  ${\rm arcsec}^{-2}$) $q_{25} = 0.51 \pm 0.06$ 2
  $q_{25} = 0.54 \pm 0.04$ 3
Asymmetry $Q_{\rm asym} = 1.7\%$ 3
Position angle (25 B mag  ${\rm arcsec}^{-2}$) PA $= 55.4\hbox{$^\circ$ }$ 2
  PA $= 62\hbox{$^\circ$ }\pm 4\hbox{$^\circ$ }$ 3
Central surface brightness $\mu_B(0) = 23.3$ mag  ${\rm arcsec}^{-2}$ 3
Apparent total B mag $B_{\rm T}=13.81 \pm 0.22$ mag 2
  $B_{\rm T}=13.8 \pm 0.1$ mag 3
Corrected apparent B mag $B_{\rm c}=13.8 \pm 0.22$ mag 2
  $B_{\rm c}=13.6 \pm 0.1$ mag 3
Corrected absolute B mag MB=-16.44 mag 2
  $M_B=-16.6 \pm 0.3 $ mag 3
Distance D=8.02 Mpc 2
  $D=10.8\pm 1.4$ Mpc 3
  D=7.7 Mpc 4
Scale $1\hbox{$^\prime$ }=2.3$ kpc 2
  $1\hbox{$^\prime$ }=3.1\pm0.4$ kpc 3
  $1\hbox{$^\prime$ }=2.2$ kpc 4
Total H I mass $M_{\rm HI}=(6.4\pm1.7)\times10^8$ ${M}_\odot$ 3
H I mass-to-blue-luminosity ratio $M_H {\sc i}/L_B=0.96\pm0.14~{M}_\odot/{L}_{B,\odot}$ 3

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