Stephanian's star : the energy distribution reveals a nontypical cataclysmic variable.
DOI: 10.1086/130856
Bibcode: 1981PASP...93..456S
Szkody, P.
Abstract
Einstein, IUE, optical multichannel spectrophotometry, and IR observations of Stepanian's star are discussed in terms of other known cataclysmics. While the X-ray flux and IUE emission-line data are similar to that of dwarf novae, the total continuum flux distribution from uv-IR is cooler (peaking near a 10,000 K blackbody) and is unlike either a stellar component or a classic steady-state disk. The IR data show no evidence for a late-type component.
1981
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Publications of the Astronomical Society of the Pacific
IUE
13