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ASCA observation of 4U1624–49
Published online by Cambridge University Press: 12 April 2016
Abstract
ASCA observations of the LMXRB 4U1624–49 reveal the presence of extended emission surrounding the X-ray source probably due to a dust scattered halo. The halo spectrum can account for the low energy excess seen in the dip spectrum.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 685 - 686
- Copyright
- Copyright © Astronomical Society of the Pacific 1997
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