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- W2029121767 abstract "Recent observations of UGC 4879 with the Advanced Camera for Surveys on the Hubble Space Telescope confirm that it is a nearby isolated dwarf irregular galaxy. We measure a distance of 1.36 ± 0.03 Mpc using the tip of the red giant branch method. This distance puts UGC 4879 beyond the radius of first turnaround of the Local Group and ∼700 kpc from its nearest neighbor Leo A. This isolation makes this galaxy an ideal laboratory for studying pristine star formation uncomplicated by interactions with other galaxies. We present the star formation history of UGC 4879 derived from simulated color–magnitude diagrams." @default.
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- W2029121767 date "2011-02-14" @default.
- W2029121767 modified "2023-09-24" @default.
- W2029121767 title "THE STAR FORMATION HISTORY OF ISOLATED DWARF UGC 4879" @default.
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