Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T20:30:12.657Z Has data issue: false hasContentIssue false
  • English
  • Français

ASCA observation of 4U1624–49

Published online by Cambridge University Press:  12 April 2016

Lorella Angelini ,
Arvind Parmar  and
Nicholas White
Lorella Angelini
Affiliation:
LHEA, Code 660, NASA/GSFC, Greenbelt, MD 20771
Arvind Parmar
Affiliation:
ESTEC/SSD/ESA, 2200 AG Noordwijk, The Netherlards
Nicholas White
Affiliation:
LHEA, Code 660, NASA/GSFC, Greenbelt, MD 20771

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Church, et al., 1995, A&A.Google Scholar
White, N.E., Nagase, F.,& Parmar, A.N. 1995, in Accretion Driven X-ray Binaries, eds. Lewin, W. & van Paradijs, J.. Cambridge University Press.Google Scholar