The Rapid X-ray Variability of Gm Sagittarii (sax J1819.3–2525 = Xte J1819–254)

We report on the rapid X-ray variability of the variable star and X-ray transient GM Sgr (SAX J1819.3–2525; XTE J1819–254) as observed on 15 Sept. 1999 by the proportional counter array (PCA) on board the Rossi X-ray Timing Explorer (RXTE). During the first ∼900 seconds of the first RXTE/PCA observation, GM Sgr showed very strong Xray fluctuations by a factor of 4 on time scales of seconds to about 500 on time scales of minutes. The spectrum of the source during this flaring episode became harder when the count rate decreased. After this flaring episode, GM Sgr entered a quiescent state in which it remained for the rest of this, and the subsequent RXTE/PCA observations. The X-ray spectrum was considerable softer in this quiescent state than during the flaring episode. The intrinsic X-ray luminosity (both during the flaring episode and the quiescent state) and the rapid X-ray variability do not strongly constrain the nature of the compact object (neutron star or black hole) in the system, although a black hole seems to be more likely. The very short duration of the bright X-ray phase of GM Sgr and its likely close distance suggest that many similar objects could be present in our galaxy, most of which are not noticed when they are in X-ray outburst due to the short duration of these outbursts. A considerable number of the black holes present in our galaxy might be contained in systems similar to GM Sgr. Subject headings: accretion, accretion disks — stars: individual (GM Sgr, SAX J1819.3–2525, XTE J1819–254) — X-rays: stars