The ratio of color excesses in UBV photometry

Details The ratio of color excesses in UBV photometry The ratio of color excesses in UBV photometry

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..425g&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, June 1975, p. 425-432. Research supported by the Universidad de Chil

Mathematics

14

Interstellar Extinction, Stellar Spectrophotometry, Ubv Spectra, Early Stars, Electromagnetic Absorption, Galactic Structure, H Lines, Luminous Intensity, Main Sequence Stars, Numerical Integration, Transformations (Mathematics)

Scientific paper

Numerical integrations have been performed in order to obtain the ratio of the color excesses in UBV photometry. The data were analyzed to study the dependence of this ratio and of the value of R on the color of the stars and on the reddening itself. The results show that the ratio of the color excesses is practically independent of the reddening, while R appears to change more with the spectral type than with the total amount of reddening.

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