Abstract
First results of high-resolution (R=50000) spectroscopic observations of B[e]-stars of the Magellanic Clouds are presented. The line profiles are compared with theoretical profiles obtained for a disk-like geometry as suggested for the B[e] -supergiants.
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Pöllitsch, G. F.: 1981, Astron. Astrophys. 97, 175
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Zickgraf, F.-J., Wolf, B., Stahl, O., Leitherer, C, Klare, G.: 1985, Astron. Astrophys. 143, 421
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© 1988 Kluwer Academic Publishers
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Zickgraf, FJ. (1988). Highly resolved emission-line profiles of B[e] -supergiants. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_18
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DOI: https://doi.org/10.1007/978-94-009-2941-8_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7824-5
Online ISBN: 978-94-009-2941-8
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