Computer Science
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236...73t&link_type=abstract
In ESA Recent Results on Cataclysmic Variables p 73-76 (SEE N86-20287 10-93)
Computer Science
2
Cataclysmic Variables, Dwarf Novae, X Ray Sources, Stellar Magnitude, Stellar Spectra, Stellar Spectrophotometry, X Ray Spectra
Scientific paper
Two X-ray emitting cataclysmic variables were discovered as a result of a program to identify faint X-ray sources located by the HEAO-A3 modulation collimator experiment. The objects, H0534-581 and 1H0542-407, have similar high excitation spectra with intense emission lines showing broad and narrow components. Photometry shows that H0534-581 and 1H0542-407 have average magnitudes of V=14.9 and 15.7 respectively, leading to Lx/Lopt ratios of 1.5 (typical of dwarf novae in quiescence). While pronounced variability of delta B or = 1.5 mag is observed from both systems, there is no clear evidence for repeatable orbital periods between 1 and 4 hr.
Bradt Hale V.
Buckley David A. H.
Remillard Ron A.
Schwartz Dana A.
Tuohy Ian R.
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