Correcting the PL Relation?

Details Correcting the PL Relation? Correcting the PL Relation?

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999iaus..192..459l&link_type=abstract

The stellar content of Local Group galaxies, Proceedings of the 192nd symposium of the International Astronomical Union held in

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3

Scientific paper

Using Cepheid photometry to determine distances, whether in the Local Group or otherwise, may require correction for metallicity differences and/or temperature differences. Calculating absolute magnitudes from Baade-Wesselink radii and photometry involves choosing one of a number of surface-brightness vs. color relations. How significant are these effects?

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