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...
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Conference item |
| Published: |
2006
|