New Results for Two Optically Faint Low Mass X-Ray Binary Systems

We present optical photometry of the low mass X-ray binary systems GX 349+2 (=X1702-363) and Ser X-1 (=X1837+049). Extensive V RI photometry of the faint optical counterpart (V = 18.4) to GX 349+2 reveals a period of 22.5 ± 0.1 h and halfamplitude 0.2 mag. This result confirms and extends our previously reported 22 h period (Wachter & Margon 1996). No color change is detected over the orbit, although the limits are modest. We also report the discovery of two new variable stars in the field of GX 349+2, including a probable W UMa system. Ser X-1 is one of the most intense persistent X-ray burst sources known. It is also one of only three burst systems for which simultaneous optical and X-ray bursts have been observed. The faint blue optical counterpart MM Ser (B ∼ 19.2) has long been known to have a companion 2.1 distant. Our images indicate that MM Ser is itself a further superposition of two stars, separated by only 1. At the very least, the ratio of inferred burst to quiescent optical flux is affected by the discovery of this additional component. In the worst case, the wrong object may have previously been assumed as the optical counterpart. Subject headings: stars: individual (GX 349+2, MM Ser) — stars: variables: other — X-rays: stars