ESO 245-G005 (HIPASS
J0145-43) is a Magellanic barred irregular galaxy at a TRGB distance
of 4.43 ± 0.45 Mpc (Karachentsev et al. 2003). It is located ~3 degrees
(200 kpc at a distance of 4 Mpc) from the spiral galaxy NGC 625 in the
outskirts of the Sculptor Group. Our ATCA HI data show a large, somewhat
warped HI disc extending well beyond the star-forming stellar body. The HI
emission is brightest near three prominent star-forming regions shown in the
multi-wavelength image by Wang et al. (2017); we observe an HI depression
towards the galaxy center. Cote et al. (2000) use ATCA HI maps to carry out
a tilted-ring analysis; they find the HI kinematical axis of ESO 245-G005 to
depart from the optical major axis. For a detailed discussion of the HI
kinematics see Kirby et al. (2012). We measure FHI = 83.2 Jy km/s,
in agreement with HIPASS (Koribalski et al. 2004). SINGG Hα (Meurer et
al. 2006) and GALEX UV (Dale et al. 2009; Wong et al. 2016) images
allow a detailed study of the galaxy's local star formation properties with
respect to the HI gas density.
Reference:
Koribalski et al. 2018
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