Discovery of a cool expanding shell at -1200 kilometers per second around V471 Tauri

Astronomy and Astrophysics – Astrophysics

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Eclipsing Binary Stars, Gas Expansion, Stellar Envelopes, Ultraviolet Spectra, Absorption Spectra, Iue, K Stars, Spectral Line Width, Stellar Winds, White Dwarf Stars

Scientific paper

High-resolution IUE spectra of V471 Tauri reveal the presence of a very-high-velocity cool expanding gas in the line of sight to the binary system with an expansion velocity of -1200 km/s. The summed strength of the coadded absorption is 125 mA + or - 25 mA, with FWHM = 30 km/s. It is suggested that the observed absorption may be related to the narrow coadded absorption at -590 km/s noted by Bruhweiler and Sion (1966). The large expansion velocity suggests a possible association with an ancient nova outburst.

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