Abstract
321 Galactic fundamental-mode Cepheids with good B, V, and (in most cases) i photometry by Berdnikov et al. (2000) and with homogenized color excesses E(B - V) based on Fernie et al. (1995) are used to determine their period-color (P-C) relation in the range of 0.4
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Tammann, G. A., Sandage, A., & Reindl, B. (2003). New period-luminosity and period-color relations of classical Cepheids: I. Cepheids in the galaxy. Astronomy and Astrophysics, 404(2), 423–448. https://doi.org/10.1051/0004-6361:20030354
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