Stepanian's star - The energy distribution reveals a nontypical cataclysmic variable

Details Stepanian's star - The energy distribution reveals a nontypical cataclysmic variable Stepanian's star - The energy distribution reveals a nontypical cataclysmic variable

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pasp...93..456s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 93, Aug.-Sept. 1981, p. 456-459.

Other

11

Eclipsing Binary Stars, Spectral Energy Distribution, Stellar Radiation, Stellar Spectra, Stellar Spectrophotometry, Variable Stars, Dwarf Novae, Dwarf Stars, Heao 2, Infrared Spectra, Iue, Late Stars, Novae, Stellar Temperature, Ubv Spectra, Ultraviolet Spectra, X Ray Spectra

Scientific paper

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.

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