THE EC-14026 STARS - VI - PG-1047+003

We report the discovery of rapid oscillations in the sdB star PG 1047 + 003. The oscillations are multiperiodic, with nine periods in the ra nge 104-162 s. The optical spectrum of PG 1047 + 003 is consistent wit h that of a single sdB star. Line profile fitting yields an effective temperature of 35000+/-1000 K and log g=5.9+/-0.1, although optical ph otometry and IUE spectrophotometry may indicate a cooler effective tem perature. These properties demonstrate that PG1047+003 is an EC 14026 star, a recently discovered class of sdB pulsators. Optical and infrar ed photometry constrains any cool companion to the sdB star to be a ma in-sequence star of spectral type MO or later. With V=13.47 and a rela tively rich pulsation spectrum, PG1047+003 is an attractive target for an intensive photometric campaign to extract more periods from the li ght curve which, along with a suitable grid of pulsation models, will probe the interior structure of the star.