IUE spectra of Feige 4, a suspected source of extreme-ultraviolet radiation

Details IUE spectra of Feige 4, a suspected source of extreme-ultraviolet radiation IUE spectra of Feige 4, a suspected source of extreme-ultraviolet radiation

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..553h&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, June-July 1982, p. 553-556.

Astronomy and Astrophysics

Astronomy

Extreme Ultraviolet Radiation, Iue, Stellar Spectra, Ultraviolet Astronomy, White Dwarf Stars, Spectral Energy Distribution, Stellar Atmospheres

Scientific paper

IUE spectra are presented for Feige 4, a DB-type white dwarf. The observed energy distribution is in good agreement with that predicted by a model atmosphere with an effective temperature of 15,500 K and having extremely low hydrogen and metal abundances. These results are evidence against Feige 4 being the source of the apparent extreme-ultraviolet signal detected by Prognoz 6.

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