Circular No. 3337 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 RS CANUM VENATICORUM D. M. Gibson and R. T. Newell, New Mexico Tech, report that RS CVn was detected with the Very Large Array on Feb. 6d06h55m UT. The observations were made at 4885 MHz using a subarray of four antennae and an integration time of 5 min. A point source located within 1" of the optical position was detected at the level of 7.2 +/- 1.6 mJy. At the distance of RS CVn this corresponds to a luminosity of 1.7 x 10**17 erg s**-1 Hz**-1, comparable with large outbursts seen previously in other RS CVn stars. This observation, when combined with other attempts to detect this object, indicates that RS CVn exhibits flaring statistics similar to other members of the class (cf. Owen and Gibson 1978, Astron. J. 83, 1488). 1979 BA H. L. Giclas, Lowell Observatory, provides the following precise positions, measured by M. L. Kantz: 1979 UT R. A. (1950) Decl. Feb. 28.21736 10 21 29.67 +34 28 48.6 Mar. 4.30208 10 15 45.95 +37 17 22.6 Improved orbital elements by C. M. Bardwell: T = 1978 Sept. 26.555 ET Peri. = 290.507 e = 0.20145 Node = 142.972 1950.0 a = 1.84316 AU Incl. = 46.695 n = 0.393876 q = 1.47186 AU P = 2.50 years 1979 ET R. A. (1950) Decl. Delta r Mag. Mar. 18 9 59.98 +44 02.7 28 9 53.67 +46 48.4 1.072 1.800 18.1 Apr. 7 9 52.55 +48 16.2 17 9 56.27 +48 49.8 1.333 1.851 18.7 27 10 04.04 +48 45.0 May 7 10 15.05 +48 11.9 1.596 1.901 19.1 17 10 28.49 +47 17.5 27 10 43.73 +46 05.8 1.843 1.949 19.5 June 6 11 00.29 +44 39.9 16 11 17.78 +43 02.0 2.065 1.994 19.7 1979 March 16 (3337) Brian G. Marsden
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