Long‐Term X‐Ray Monitoring of 1E 1740.7−2942 and GRS 1758−258

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Abstract
We report on long-term observations of the Galactic bulge black hole candidates 1E 1740.7-2942 and GRS 1758-258 made with the Rossi X-Ray Timing Explorer; 1E 1740.7-2942 has been observed 77 times and GRS 1758-258 has been observed 82 times over the past 1000 days. The flux of each object has varied by no more than a factor of 2.5 during this period, and the indices of the energy spectra have varied by no more than 0.4. The power spectra are similar to other black hole candidates: flat-topped noise, breaking to a power law. Each object has exhibited a brightening that lasted for several months, and we have a found a time lag between the photon power-law index and the count rate. In both sources, the spectrum is softest during the decline from the brightening. This behavior can be understood in the context of thin-disk and advection-dominated accretion flows coexisting over a wide range of radii, with the implication that both sources have low-mass companions and accrete via Roche lobe overflow.
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