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The Astrophysical Journal
Article . 1993 . Peer-reviewed
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https://dx.doi.org/10.1086/172...
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Hubble Space Telescope spectra of the phase-modulated wind in the SMC O+WR binary R31

descriptionPublicationkeyboard_double_arrow_right Article 01 Jun 1993 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 410, page 803 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: J. B. Hutchings; L. Bianchi; S. C. Morris;

doi: 10.1086/172797

Hubble Space Telescope spectra of the phase-modulated wind in the SMC O+WR binary R31

Abstract

We present HST/GHRS profiles of C IV 1500 A at conjunction phases 0.21, 0.26, and 0.72 of the 6.5 day O6+WN3 binary R31 in the SMC. We also use IUE archival data covering other orbital phases, There are strong changes in the line profile, depending on the line of view through an ionization bubble near the WR star. We fit a model for the stellar wind and discuss the unique probe of mass loss found in this system. We also discuss the strong interstellar components of the line arising in the Galactic foreground and in the SMC.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
5
Average
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Average
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