Unravelling the Source of UV Emission in EF Eridani

Details Unravelling the Source of UV Emission in EF Eridani Unravelling the Source of UV Emission in EF Eridani

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1314..206c&link_type=abstract

INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink's 65th Birthday. AIP Conference Proceedings, Volume 1314, p

Astronomy and Astrophysics

Astronomy

White Dwarfs, Accretion Disks, Telescopes, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Accretion And Accretion Disks, Astronomical And Space-Research Instrumentation

Scientific paper

Oribital phase-resolved spectra of EF Eri were obtained with the Solar Blind Channel on the Hubble Space Telescope during its low state. The specta peaked at 1500 and 1700 A˚, and the integrated UV light curves displayed quasi-sinusoidal modulations. WD hotspot and cyclotron emission models were computed in an attempt to fit the spectroscopic morphology throughout the orbit.

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