UBV(RI)c observations for 13 bright Cepheids

Details UBV(RI)c observations for 13 bright Cepheids UBV(RI)c observations for 13 bright Cepheids

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.255..486s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, April 1, 1992, p. 486-494. Research supported by U

Astronomy and Astrophysics

Astronomy

24

Cepheid Variables, Light Curve, Stellar Spectrophotometry, Ubv Spectra, Astronomical Photometry, Radial Velocity

Scientific paper

Photometry in the UBV(RI)c system has been obtained for 13 of the brightest Cepheids in the southern sky available to the new Sydney University Stellar Interferometer. The stars observed were Eta Aq1, 1 Car, U Car, AX Cir, Beta Dor, Zeta Gem, T Mon, Kappa Pav, U Sgr, W Sgr, X Sgr, Y Sgr, and AH Vel. The main purpose of the photometry is to provide current epoch data for the phases of the variables, although for several of the stars these data are also the first in the (RI)c system.

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