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...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy: Bandyopadhyay, R, Gosling, A, Blundell, K, Podsiadlowski, P, Eikenberry, SE, Mikles, V, Miller-Jones, J, Bauer, F
Format: Journal article
Język:English
Wydane: 2006