Monitoring the winds of hot stars with HST/GHRS

Details Monitoring the winds of hot stars with HST/GHRS Monitoring the winds of hot stars with HST/GHRS

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221...87h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 87-94

Astronomy and Astrophysics

Astronomy

Main Sequence Stars, O Stars, Stellar Physics, Stellar Winds, Ultraviolet Astronomy, Ultraviolet Spectra, High Resolution, Hubble Space Telescope, Spaceborne Astronomy, Spectroscopy, Stellar Evolution

Scientific paper

We present observations obtained with the Goddard High Resolution
spectrograph (GHRS) of three O-type stars: xi per (O7 III), lambda Cep
(O6 Iaf) and 10 Lac (O9 V). These observations show evidence of
instabilities in the winds of all three stars, although not necessarily
those expected from current models of structured winds.

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