New Cepheid distances to nearby galaxies based on BVRI CCD photometry. III - NGC 300

Astronomy and Astrophysics – Astronomy

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Astronomical Photometry, Cepheus Constellation, Charge Coupled Devices, Local Group (Astronomy), Red Shift, Astrometry, Hubble Constant, Interstellar Extinction, Spiral Galaxies

Scientific paper

A true distance modulus of (m - M)0 = 26.66 +/- 0.10 mag (corresponding to 2.1 +/- 0.1 Mpc) has been determined for the Sculptor Group spiral galaxy NGC 300. New CCD data have been obtained for a sample of known Cepheids in this galaxy from which apparent distance moduli at B, V, R, and I wavelengths are determined. Combining the data available at different wavelenghts, and assuming a true distance modulus to the LMC of 18.5 mag, a true distance modulus is obtained for NGC 300, corrected for the effects of interstellar reddening. The availability of a new distance to NGC 300 brings to five the total number of galaxies with new CCD photometry of Cepheids, useful for calibration of the Hubble constant.

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