KK258, a new transition dwarf galaxy neighbouring the Local Group

preprint2014arXivOpen access

Abstract

Here we present observations with the Advanced Camera for Surveys on the Hubble Space Telescope of the nearby, transition-type dwarf galaxy KK258 = ESO468-020. We measure a distance of 2.23±\pm0.05 Mpc using the Tip of Red Giant Branch method. We also detect Hαα emission from this gas-poor dwarf transition galaxy at the velocity VhV_h = 92±\pm5 km s−1^{-1} or VLGV_{LG} = 150 km s−1^{-1}. With this distance and velocity, KK258 lies near the local Hubble flow locus with a peculiar velocity ∼\sim3 km s−1^{-1}. We discuss the star formation history of KK258 derived from its colour-magnitude diagram. The specific star formation rate is estimated to be log[sSFR] = −2.64-2.64 and −2.84-2.84 (Gyr−1^{-1}) from the FUV-flux and Hαα-flux, respectively. KK258 has the absolute magnitude MB=−10.3M_B = -10.3 mag, the average surface brightness of 26.0 mag arcsec−2^{-2} and the hydrogen mass log(MHI)<5.75M⊙{\rm log}(M_{HI}) < 5.75 M_\odot. We compare KK258 with 29 other dTr- galaxies situated within 5 Mpc from us, and conclude that its properties are typical for transition dwarfs. However, KK258 resides 0.8 Mpc away from its significant neighbour, the Sdm galaxy NGC 55, and such a spatial isolation is unusual for the local transition dwarfs.

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