The reddening of Beta Doradus

Astronomy and Astrophysics – Astronomy

Scientific paper

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A Stars, B Stars, Cepheid Variables, Red Shift, Stellar Spectrophotometry, Ubv Spectra, Interstellar Extinction, Stellar Luminosity

Scientific paper

New UBV photometry for B and A-type stars within 1 1/2 deg of the 9.84 d Cepheid Beta Dor is combined with spectroscopic data to derive the distance-reddening relation for stars in this region. The inferred color excess of Beta Dor is E(B-V) = 0.07 plus or minus 0.025, in agreement with the value obtained by Dean et al. (1978) using their Cepheid intrinsic color relation.

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