Determining the nature of the faint X-ray source population near the Galactic Centre
We present results of a multi-wavelength program to study the faint discrete X-ray source population discovered by Chandra in the Galactic Centre (GC). From IR imaging obtained with the VLT we identify candidate K-band counterparts to 75% of the X-ray sources in our sample. By combining follow-up VL...
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| Materiálatiipa: | Conference item |
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2006
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