Far Ultraviolet Spectroscopic Explorer Spectroscopy of the O VI Resonance Doublet in Sand 2 (WO)

Astronomy and Astrophysics – Astronomy

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Stars: Evolution, Stars: Individual: Alphanumeric: Sand 2, Stars: Wolf-Rayet

Scientific paper

We present Far Ultraviolet Spectroscopic Explorer spectroscopy of Sand 2, an LMC WO-type Wolf-Rayet star, revealing the O VI resonance P Cygni doublet at 1032-1038 Å. These data are combined with Hubble Space Telescope Faint Object Spectrograph ultraviolet and Mount Stromlo 2.3 m optical spectroscopy and analyzed using a spherical, non-LTE, line-blanketed code. Our study reveals exceptional stellar parameters: T*~150,000 K, v∞=4100 km s-1, log(L/Lsolar)=5.3, and M=1×10-5 Msolar yr-1, if we adopt a volume filling factor of 10%. Elemental abundances of C/He~0.7+/-0.2 and O/He~0.15+0.10-0.05 by number qualitatively support previous recombination line studies. We confirm that Sand 2 is more chemically enriched in carbon than LMC WC stars and that it is expected to undergo a supernova explosion within the next 5×104 yr.

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