NASA NTRS · 19800056477
Mass loss from O-type stars
Abstract
We determine mass loss rates for six O-type stars from the violet-shifted absorption profile of the resonance C IV and N V lines, using the IUE satellite and the high-resolution camera. The values are substantially below those of Of stars (which have optical emission lines) of similar luminosity.
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Conti, P. S., Garmany, C. D.. 1980-05-15. Mass loss from O-type stars. https://ntrs.nasa.gov/citations/19800056477
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