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IR contamination in quiescence X-Ray Novae
Published online by Cambridge University Press: 01 August 2006
Abstract
We present archival optical-IR observations of a number of short period X-ray novae (XRNe). We use these to show that in contrast to the current paradigm, there is likely significant non stellar flux in the infra-red (IR).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 435 - 436
- Copyright
- Copyright © International Astronomical Union 2007