X-ray, optical and UV observations of the AM HER system E2003 + 225

Details X-ray, optical and UV observations of the AM HER system E2003 + 225 X-ray, optical and UV observations of the AM HER system E2003 + 225

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..151m&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Stellar Mass Accretion, Stellar Spectra, Ultraviolet Spectra, White Dwarf Stars, X Ray Spectra, Bremsstrahlung, Cyclotron Radiation, Exosat Satellite, Gratings (Spectra)

Scientific paper

The AM Her type object E2003 + 225 was observed with Exosat, IUE and ground-based telescopes on Oct. 12, 1983. The brightness of the ultrasoft X-ray component allowed the Objective Grating Spectrometer (OGS) to be used, which gave a model-independent determination of the temperature of the blackbody spectrum. The star was observed again on July 24, 1984 by IUE with simultaneous optical spectrophotometry. The high resolution of this observation revealed complex line profiles, and a systematic velocity much smaller than previously reported. The composite energy distribution is presented.

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