Deep Infrared Imaging of the Microquasars 1E1740-2942 and GRS 1758-258

Abstract

We present deep infrared ($2.2\mu$m) imaging of the Galactic microquasars 1E1740-2942 and GRS 1758-258 using the Keck-I 10-meter telescope in June 1998. The observations were taken under excellent seeing conditions ($\sim 0.45 \arcsec$ full-width half-maximum), making them exceptionally deep for these crowded fields. We used the USNO-A2.0 catalog to astrometrically calibrate the infrared images (along with an optical CCD image in the case of GRS 1758-258), providing independent frame ties to the known radio positions of the objects. For 1E1740-2942, we confirm potential candidates for the microquasar previously identified by Marti et al., and show that none of the objects near the microquasar have varied significantly from 1998 to 1999. For GRS 1758-258, our astrometry indicates a position shifted from previous reports of candidates for the microquasar. We find no candidates inside our 90% confidence radius to a $2\sigma$ limiting magnitude of $K_s=20.3$ mag. We discuss the implications of these results for the nature of the microquasar binary systems.

To appear in the Astrophysical Journal; 15 pages, including 4 figures

Cited by in corpus (13)

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• Chandra imaging spectroscopy of 1E 1740.7 - 2942
• Identification of the optical and near-infrared counterpart of GRS 1758-258
• Chandra High Resolution Camera Imaging of GRS 1758-258
• Suzaku Observations of the Galactic Center Microquasar 1E 1740.7-2942
• Suzaku Observations of the Great Annihilator and the Surrounding Diffuse Emissions
• The broad band X-ray spectrum of the black hole candidate GRS1758-258
• Effects of precession versus instabilities on the jets of GRS 1758-258