Other
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..338s&link_type=abstract
CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3
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1
Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, X-Ray Binaries, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Eclipsing Binaries, Spectroscopic Binaries, Close Binaries
Scientific paper
An analysis of the color indices and absolute magnitudes MV0 of the super-soft X-ray (SSX) binary sources (including the V Sge-type stars) and classical novae in the SSX phase is presented. It can help comparing the properties and configuration of the reprocessing medium in the individual systems. The (U - B)0 and (B - V)0 colors of the novae in SSX phase are similar to those of the classical SSX binaries, but display a larger scatter for the individual objects. The range of MV0 of the individual objects with SSX emission is very large, from MV0 = 8.5 to MV0 = -4. The SSX phase of the novae V 1974 Cyg and V 382 Vel occurred at significantly brighter MV0 than of most SSX binaries while MV0 of U Sco was comparable to the SSX binaries. The implications for the reprocessing medium are given.
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