Space reddenings for six Cepheid variables

Details Space reddenings for six Cepheid variables Space reddenings for six Cepheid variables

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jrasc..78..229t&link_type=abstract

Journal of the Royal Astronomical Society of Canada (ISSN 0035-872X), vol. 78, Dec. 1984, p. 229-240. Research supported by the

Other

15

Cepheid Variables, Interstellar Extinction, Star Clusters, Astronomical Photometry, F Stars, Star Distribution, Ubv Spectra

Scientific paper

Color excesses are derived for six galactic Cepheids from reddenings found for neighboring stars which seem likely to be physically associated with each variable. The Cepheids studied are: SU Cas, which is associated with a dust complex and R association; Zeta Gem and Alpha UMi, which have F dwarfs as close companions; BB Sgr and SZ Tau, which lie in the coronal regions of the clusters Collinder 394 and NGC 1647, respectively; and SV Vul, which is involved in an older region of the association Vul OB1. The derived reddenings are in good agreement with other, independent, estimates from the literature.

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