Determining the nature of the faint X-ray source population near the Galactic Centre

Determining the nature of the faint X-ray source population near the Galactic Centre

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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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मुख्य लेखकों: Bandyopadhyay, R, Gosling, A, Blundell, K, Podsiadlowski, P, Eikenberry, SE, Mikles, V, Miller-Jones, J, Bauer, F
स्वरूप: Conference item
प्रकाशित: 2006
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