Deep Stellar Photometry of IC 10

Details Deep Stellar Photometry of IC 10 Deep Stellar Photometry of IC 10

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999iaus..192..244t&link_type=abstract

The stellar content of Local Group galaxies, Proceedings of the 192nd symposium of the International Astronomical Union held in

Astronomy and Astrophysics

Astronomy

7

Scientific paper

A deep R,I CCD photometry is presented, based on 6-m telescope frames taken to the east star complex of IC 10. The CM diagram show an existence of blue and red supergiants and red giant branch. The distance modulus estimated from TRGB is (m-M)I = 24.8 ± 0.1. The luminosity function of brightest stars and the integrated magnitudes of the complex are obtained. The masses and ages of brightest stars are derived from comparisons with theoretical evolutionary tracks.

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