Cepheids and Long-Period Variables in NGC 4395

@article{Thim2004CepheidsAL,
  title={Cepheids and Long-Period Variables in NGC 4395},
  author={F. Thim and J. Hoessel and A. Saha and J. Claver and A. Dolphin and G. N. O. A. Observatory and U. Wisconsin--Madison and Astronomisches Institut der Universitaet Basel},
  journal={The Astronomical Journal},
  year={2004},
  volume={127},
  pages={2322-2343}
}
Repeated imaging observations of NGC 4395 were made with the WIYN 3.5 m and the KPNO 2.1 m telescopes. From the photometry of the resolved brighter stars in this galaxy, 11 Cepheids with periods ranging between 12 and 90 days have been identified. The true distance modulus has been derived from the apparent distance moduli in g, r, and i. The distance modulus is 28.02 ± 0.18 based on the LMC period-luminosity (P-L) relation of Sandage, Reindl, & Tammann; this corresponds to a distance of 4.0… Expand
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