UGC 8565, VV 828, Mrk 1479, SBS 1332+518, I Zw 64, KPG 384
NGC 5238 is an irregular galaxy[5] in the constellation Canes Venatici. Located at a comoving distance of 4.51 Mpc,[4] it is 64.4 arcseconds in diameter.[8] It has sometimes been classified as a blue compact dwarf galaxy.[9] Although some authors have hypothesized it to be a member of the M101 Group of galaxies, it is currently believed to be an isolated galaxy.[10]
At an inclination of 39° with respect to Earth,[3] NGC 5238 has a total mass of 117 million solar masses,[6] with a star formation rate of 0.01 solar masses per year.[11] Of the total mass, HI gas appears to account for 26 million solar masses.[3]
^Gyulzadyan, M. V.; Stepanian, J. A.; Petrosian, A. R.; Kunth, D.; McLean, B.; Comte, G. (2003). "Spectroscopic Study of a Large Sample of Galaxies Discovered in the Second Byurakan Survey Fields". Astrophysics (English Translation of Astrofizika). 46 (2): 131. Bibcode:2003Ap.....46..131G. doi:10.1023/A:1024011318696. S2CID118938315.
^Huchtmeier, W. K.; Richter, O.-G. (1988). "H I observations of galaxies in the Kraan-Korteweg-Tammann catalogue of nearby galaxies. III - Global parameters of the galaxies". Astronomy and Astrophysics. 203: 237. Bibcode:1988A&A...203..237H.
^ abCite error: The named reference Spitzer was invoked but never defined (see the help page).