New Period-Luminosity and Period-Color relations of classical Cepheids: I. Cepheids in the Galaxy

321 Galactic fundamental-mode Cepheids with good B, V, and (in most cases) I photometry by Berdnikov et al. ([CITE]) and with homogenized color excesses $E(B-V)$ based on Fernie et al. ([CITE]) are used to determine their period-color (P-C) relation in the range $0.4

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2003-06, Vol.404 (2), p.423-448
Main Authors: Tammann, G. A., Sandage, A., Reindl, B.
Format: Article
Language:English
Subjects:
Cepheids
cosmological parameters
distance scale
Magellanic Clouds
supernovae: general
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Description
Summary:321 Galactic fundamental-mode Cepheids with good B, V, and (in most cases) I photometry by Berdnikov et al. ([CITE]) and with homogenized color excesses $E(B-V)$ based on Fernie et al. ([CITE]) are used to determine their period-color (P-C) relation in the range $0.4
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:20030354