BVI photometry of Galactic Cepheids (Tammann+, 2003)

Details BVI photometry of Galactic Cepheids (Tammann+, 2003) BVI photometry of Galactic Cepheids (Tammann+, 2003)

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34040423t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/404/423. Originally published in: 2003A&A...404..423T

Physics

Stars: Variable, Photometry: Ubvri

Scientific paper

321 Galactic fundamental-mode Cepheids with good B,V,I photometry by Berdnikov et al. (2000, Cat. ) and with homogenized color excesses E(B-V) based on Fernie et al. (1995IBVS.4148....1F) are used to determine their period-colour relation in the range 0.4B=4.17, RV=3.17, and RI=1.89. The two sets define two independent P-L relations which agree very well in slope. They are therefore combined into a single mean Galactic P-L relation.
(1 data file).

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