Conclusions The spectra obtained with FUSE, HST, and HUT represent qualitative improvements over those that could be obtained with IUE. For the high ... Long, K.S., Knigge, C. Modeling the spectral signatures of accretion disk winds: a new monte carlo approach. ... E.M., Gansicke, B.T., Szkody, P. WZ Sge: HST spectroscopy of the cooling of the WD after the 2001 Outburst. ApJ 602. 948-959. 2004.
|Title||:||Spectra and timing of compact X-ray binaries|
|Author||:||Pranab Ghosh, Edward Peter Jacobus van den Heuvel|