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The Properties of Population I WO Stars

Published online by Cambridge University Press:  03 August 2017

R. L. Kingsburgh  and
M. J. Barlow
R. L. Kingsburgh
Affiliation:
Department of Physics & Astronomy University College London Gower St., London. WC1E 6BT.
M. J. Barlow
Affiliation:
Department of Physics & Astronomy University College London Gower St., London. WC1E 6BT.

Abstract

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High and low resolution UV and optical spectra of the four Population I WO stars originally classified by Barlow and Hummer (1982), Sanduleak 1, 2, 4 and 5, have been analyzed. Reddenings, terminal velocities and the relative abundances of He2+, C4+ and O6+ have been determined. The results are presented in Table 1.

Type
Session II. Atmospheres
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 101
Copyright
Copyright © Kluwer 1991