* Astronomy

Title: The structural properties and star formation history of Leo T from deep LBT photometry
Authors: J. T. A. de Jong, J. Harris, M. G. Coleman, N. F. Martin, E. F. Bell, H-W. Rix, J. M. Hill, E. D. Skillman, D. J. Sand, E. W. Olszewski, D. Zaritsky, D. Thompson, E. Giallongo, R. Ragazzoni, A. DiPaola, J. Farinato, V. Testa, J. Bechtold
(Version v2)

We present deep, wide-field g and r photometry of the transition type dwarf galaxy Leo T, obtained with the blue arm of the Large Binocular Telescope. The data confirm the presence of both very young (<1 Gyr) as well as much older (>5 Gyr) stars. We study the structural properties of the old and young stellar populations by preferentially selecting either population based on their colour and magnitude. The young population is significantly more concentrated than the old population, with half-light radii of 104+-8 and 148+-16 pc respectively, and their centres are slightly offset. Approximately 10% of the total stellar mass is estimated to be represented by the young stellar population. Comparison of the colour-magnitude diagram (CMD) with theoretical isochrones as well as numerical CMD-fitting suggest that star formation began over 10 Gyr ago and continued in recent times until at least a few hundred Myr ago. The CMD-fitting results are indicative of two distinct star formation bursts, with a quiescent period around 3 Gyr ago, albeit at low significance. The results are consistent with no metallicity evolution and [Fe/H] ~ -1.5 over the entire age of the system. Finally, the data show little if any sign of tidal distortion of Leo T.

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