The very short period Cepheid (RR Lyr) variables. 2: Light and color curves of variables in the solar vicinity

Details The very short period Cepheid (RR Lyr) variables. 2: Light and color curves of variables in the solar vicinity The very short period Cepheid (RR Lyr) variables. 2: Light and color curves of variables in the solar vicinity

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....107.1834e&link_type=abstract

The Astronomical Journal, vol. 107, no. 5, p. 1834-1849

Astronomy and Astrophysics

Astronomy

8

Astronomical Catalogs, Astronomical Photometry, Cepheid Variables, Light Curve, Lyra Constellation, Electrophotometers, H Beta Line, Optical Filters, Reflecting Telescopes, Tables (Data)

Scientific paper

Four color and H beta observations for 43 very short period Cepheids (VSPC, RRLyr) variables have been obtained with the Cerro Tololo and Kitt Peak reflectors. The color systems are defined in Eggen (1982). Contemporary, photo-electric V-light curves have been used to establish the phasing and the resulting periods used to compute the phases for the present observations. These phases are then adjusted to fit the V-light curves and the resulting periods and adjusted phases are given.

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