COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2706 Konkoly Observatory Budapest 15 April 1985 HU ISSN 0374 - 0676 COMPARISON STARS FOR SOME ECLIPSING BINARIES As part of a continuing photometric program of mostly long-period interacting eclipsing binaries, comparison and check stars have been observed for constancy. Observations were made with u,v,b,y, and I intermediate-band filters, and transformed to the standard Stromgren-Crawford and Kron systems. Most observations were made with the 1-m Prairie reflector located at the Mount Laguna Observatory. All were made with a pulse-counting photometer with refrigerated RCA 31034A-02 photomultiplier. TABLE I Constant Comparison and Check Stars Binary Comparison Star Check Star n AQ Cas + 61deg 223 +62deg 229 6 RS Cep + 80deg 156 +79deg 159 12 RZ Cnc + 31deg 1848 +31deg 1857 7 KU Cyg + 46deg 2879 1 26 RX Gem + 33deg 1417 +33deg 1421 6 AU Mon - 01deg 1413 -01deg 1446 7 RZ Oph + 06deg 3917 +06deg 3918 24 DN Ori + 10deg 973 +09deg 1016 3 RW Per + 42deg 938 +41deg 844 21 RZ Sct - 08deg 4606 -08deg 4605 10 RW Tau + 27deg 628 +27deg 618 3 1 Star 'd', Popper (1964) TABLE II Non-Constant Stars Binary Star AQ Cas +61deg 240 RS Cep +80deg 159 RZ Cnc +32deg 1776 TABLE III Comparison Star Colors Comparison to: (V-I) (b-y) (v-y) (u-b) n AQ Cas 0.294 +/- 0.005 0.279 +/- 0.004 0.688 +/- 0.004 1.313 +/- 0.005 1 RS Cep -0.130 +/- 0.007 0.047 +/- 0.003 0.242 +/- 0.005 1.462 +/- 0.014 4 RZ Cnc 1.052 +/- 0.013 0.777 +/- 0.003 2.149 +/- 0.006 3.206 +/- 0.009 6 KU Cyg 1.008 +/- 0.017 0.729 +/- 0.005 1.823 +/- 0.016 2.730 +/- 0.020 5 RX Gem -0.234 +/- .023 0.000 +/- 0.002 0.123 +/- 0.003 0.964 +/- 0.005 3 AU Mon -0.143 +/- 0.005 0.027 +/- 0.008 0.181 +/- 0.008 1.269 +/- 0.008 2 RZ Oph 0.520 +/- 0.006 0.415 +/- 0.004 1.034 +/- 0.005 1.700 +/- 0.008 11 DN Ori 0.014 +/- 0.010 0.095 +/- 0.017 0.396 +/- 0.012 1.629 +/- .012 1 RW Per 0.348 +/- 0.005 0.315 +/- 0.006 0.773 +/- 0.009 1.437 +/- 0.012 3 RZ Sct (:) 0.184 +/- 0.004 0.442 +/- 0.011 1.678 +/- 0.005 2 RW Tau -0.067(:) 0.088 +/- 0.026 0.310 +/- 0.024 1.484 +/- 0.027 3 Those binaries whose comparison and check stars were constant at all observed wavelengths to better than 0.01 mag. are listed in Table I. The last column gives the number of nights on which comparison/check star observations were made. Table II lists other stars, close to three binaries, which are variable with amplitude > 0.01 mag. Colors of the constant comparison stars of Table I were found for those nights on which more than a dozen standard stars were observed. These results are given in Table III. Transformation equations for (v-y) and (u-b) are (Olson, 1981): (v-y) = P + I' C (cl) + RC (vy) (u-b) = L' + J" C (cl) + M' C (ub). The author thanks the U.S. National Science Foundation for continuing support of his program on interacting binaries, and the Director and Staff of the Mount Laguna Observatory for support and assistance. EDWARD C. OLSON Department of Astronomy, University of Illinois 1011 W. Springfield Urbana, IL 61801-3000 References: Olson, E. C. 1981, Publ. Astron. Soc. Pacific 93, 783. [BIBCODE 1981PASP...93..783O ] Popper, D. M. 1964, Astroph. J. 139, 143. [BIBCODE 1964ApJ...139..143P ]