2005MNRAS.360..185B

We present V and I photometry of a 9.4x9.4 arcmin² field centred on the dwarf spheroidal galaxy Leo II. The tip of the red giant branch (TRGB) is identified at I^TRGB= 17.83±0.03 and adopting <[M/H]≥-1.53 ±0.2 from the comparison of RGB stars with Galactic templates, we obtain a distance modulus (m-M)₀= 21.84±0.13, corresponding to a distance D= 233±15 kpc. Two significant bumps have been detected in the luminosity function of the RGB. The fainter bump (B1, at V= 21.76±0.05) is the RGB bump of the dominant stellar population while the actual nature of the brightest one (B2, at V= 21.35±0.05) cannot be firmly assessed on the basis of the available data; it may be due to the asymptotic giant branch clump of the main population or it may be a secondary RGB bump. The luminosity of the main RGB bump (B1) suggests that the majority of RGB stars in Leo II belong to a population that is ≳4 Gyr younger than the classical Galactic globular clusters. The stars belonging to the He-burning red clump are shown to be significantly more centrally concentrated than RR Lyrae and blue horizontal branch stars, probing the existence of an age/metallicity radial gradient in this remote dwarf spheroidal.