Bibcode
Sanna, N.; Bono, G.; Monelli, M.; Drozdovsky, I.; Giuffrida, G.; Cassisi, S.; Pietrinferni, A.; Stetson, P. B.; Buonanno, R.; Caputo, F.; Corsi, C. E.; Ferraro, I.; Iannicola, G.; Pulone, L.
Bibliographical reference
Memorie della Società Astronomica Italiana, v.80, p.79 (2009)
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2009
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0
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Description
We present preliminary results of a photometric investigation on IC10
using data collected with ACS@HSTS and WFPC2@HST. We estimate the
distance using the Tip of the Red Giant Branch (TRGB). According to
current estimates, IC10 seems to be a member of the M31 group. By
assuming the same distance for the two different pointings, the
reddening shows a significant decrease when moving from the center
toward the external regions. Moreover, we show that stellar isochrones
at fixed metal content, distance and reddening account for both Main
Sequence (MS) and evolved stellar components.