Distances to the galaxies M81 and NGC 2403 from CCD I band photometry of Cepheids

Astronomy and Astrophysics – Astrophysics

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Astronomical Photometry, Cepheid Variables, Spiral Galaxies, Charge Coupled Devices, Error Analysis, Magellanic Clouds, Northern Hemisphere

Scientific paper

Photometric observations of two Cepheids in M81 and eight Cepheids in NGC 2403, obtained in the I band using prime-focus CCD cameras on the 3.6-m Canada-France-Hawaii Telescope and the 4.0-m telescope at KPNO during January 1988, are reported. The data are presented in tables and a period-luminosity plot and discussed in detail. The apparent I-band and true (upper-limit) distance moduli for M81 are calculated as 27.64 + or - 0.09 mag and 27.59 + or - 0.31, respectively; the corresponding values for NGC 2403 are 27.57 + or - 0.14 mag and 27.51 + or - 0.24 mag, respectively; the true moduli are equivalent to distances of 3.3 + or - 0.5 Mpc for M81 and 3.2 + or - 0.4 Mpc for NGC 2403.

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