Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apjs...41...97d&link_type=abstract
Astrophysical Journal Supplement Series, vol. 41, Sept. 1979, p. 97-117.
Astronomy and Astrophysics
Astrophysics
69
Cepheid Variables, Electrophotometry, Semiregular Variable Stars, Stellar Spectrophotometry, Abundance, Color-Color Diagram, Cyanides, Gravity Waves, Interstellar Extinction, Metallic Stars, Stellar Atmospheres, Stellar Gravitation, Stellar Luminosity, Stellar Mass, Stellar Temperature, Ubv Spectra
Scientific paper
Results are presented for DDO and UBV photoelectric photometry of 52 RV Tau and semiregular variables and candidates. CN abundances, effective temperatures, surface gravities, absolute visual magnitudes, and mass estimates are derived in the framework of the spectroscopic groupings proposed by Preston et al. (1963). The photometry suggests a further division of Preston's group A, and a possible physical connection is indicated between this group and the semiregular variables. The spectroscopic groups are shown to be well separated in the DDO color-color diagrams when mean colors are used for individual stars. An upper limit of about 3 solar masses is determined for stars in each group. A correlation between derived iron abundances and published IR excesses obtained from flux measurements at 3.6 and 11.3 microns is found which supports the contention that dust production in circumstellar shells increases with increasing metallicity.
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