COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3149 Konkoly Observatory Budapest 19 February 1988 HU ISSN 0374-0676 A NEW EPHEMERIS FOR RW ARIETIS The main purpose of this note is to establish new light elements for the variable star RW Arietis and put in agreement the photoelectric observations performed by Bookmyer et al. (1977) and Penston (1972). Such a problem is accessible if we do not take into consideration the photoelectric observations from JD 2439384, 2439505, 2439507, 2440335 and 2440337. These last observations could be influenced by an unknown cause. Figure 1 shows the common light curve of RW Arietis plotted with the newly derived ephemeris JDmax = 2439475.6618 + 0.3543145d E. Here dots and open circles represent Bookmyer's et al. (1977) and Penston's (1972) observations, respectively. The ephemeris determined above agrees with Detre's (1937) observations, as we can see in the following table. Max. hel. E O-C 2428000+ 074.550 -32178 +0d020 154.273 -31953 + .022 181.203 -31877 + .025 183.299 -31871 - .005 407.603 -31238 + .018 408.622 -31235 - .026 431.649 -31170 - .030 455.419 -31103 +0.001 The available observational data taken here into consideration seem to agree with the old proposal that RW Arietis is an RR Lyrae variable of type c in Bailey's classification. [FIGURE 1] I. TODORAN Centre for Astronomy and Space Sciences Astronomical Observatory Cluj-Napoca, Romania References Bookmyer, B.B., Fitch, W.S., Lee, T.A., Wisniewski, W.Z., Johnson, H.L., 1977, Rev. Mexicana Astron. Astrofisica 2, 235. [BIBCODE 1977RMxAA...2..235B ] Detre, L., 1937, Astron. Nachr. 262, 81. [BIBCODE 1937AN....262...81D ] Penston, M.J., 1972, Mon. Not. Roy. Astron. Soc. 156, 103. [BIBCODE 1972MNRAS.156..103P ]