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High resolution spectroscopy at the ESO 50 cm telescope: spectroscopic monitoring of luminous hot stars
Published online by Cambridge University Press: 26 May 2016
Abstract
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Galactic Luminous Blue Variables and A- and B-type supergiants were monitored spectroscopically with high resolution in wavelength and time. Line profile variations on different timescales are found.
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- 7. OB Stellar Winds
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- Copyright © Kluwer 1994
References
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Stahl, O., Wolf, B., Gäng, Th., Gummersbach, C.A., Kaufer, A., Kovacs, J., Mandel, H., Szeifert, Th.: 1993, A&A, 274, L29–L32
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Wolf, B., Mandel, H., Stahl, O., Kaufer, A., Gäng, Th., Gummersbach, C.A., Szeifert, Th.: 1993, “High resolution spectroscopy at the ESO 50 cm telescope”: The ESO Messenger
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