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The Hopkins Ultraviolet Telescope Far-Ultraviolet Spectral Atlas of Wolf-Rayet Stars

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© 1995. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Regina E. Schulte-Ladbeck et al 1995 ApJ 454 L51 DOI 10.1086/309766

1538-4357/454/1/L51

Abstract

During the 1995 March, 16 day Astro-2 mission of the Astro Space Shuttle observatory, we obtained far-UV spectra of the four WN stars WR 6 (WN5), WR 134 (WN6), WR 24 (WN7+a), and WR 40 (WN8) with the Hopkins Ultraviolet Telescope (HUT). These data, extending from 820 to 1840 Å at a resolution of ~3 Å, form the basis for the first systematic exploration of Wolf-Rayet star spectra from 1150 Å to the Lyman limit. We identify the prominent emission lines in this spectral region and discuss their changes along the WN sequence. The spectrum of HD 5980, a former WN3 + WN4.5 SMC binary recently recognized as a luminous blue variable, is classified WN6/WN8 in the UV using the WN sequence. A previously unpublished spectrum of WR 48 (WC6 + O9.5 I), obtained with HUT during the 1990 December Astro-1 mission, allows for a comparison of the WN sequence with one WC spectrum.

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10.1086/309766