Spectrophotometry of dwarf novae in the wavelength range 1250-7500 A

Details Spectrophotometry of dwarf novae in the wavelength range 1250-7500 A Spectrophotometry of dwarf novae in the wavelength range 1250-7500 A

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..185b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Jan. 1980, p. 185-194.

Astronomy and Astrophysics

Astronomy

91

Binary Stars, Dwarf Stars, Novae, Stellar Spectrophotometry, Ultraviolet Photometry, Visual Photometry, Continuous Spectra, G Stars, Stellar Mass Accretion, Stellar Models, Stellar Radiation, Stellar Spectra, Ultraviolet Astronomy

Scientific paper

The paper presents spectrophotometric observations of three southern dwarf novae BV Cen, EX Hya and VW Hyi in the wavelength range 1250-7500 A. BV Cen and EX Hya were observed in quiescence and VW Hyi on the decline from outburst. The received energy flux for BV Cen peaks at visible wavelengths, where the spectrum of a late G-star is evident. Both EX Hya and VW Hyi radiate strongly in the ultraviolet, and their continuum spectra are consistent with those predicted by steady accretion disk models.

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