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.
References
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Pöllitsch, G. F.: 1981, Astron. Astrophys. 97, 175
Wolf, B., Stahl, O.: 1985, Astron. Astrophys. 148, 412
Zickgraf, F.-J., Wolf, B., Stahl, O., Leitherer, C, Klare, G.: 1985, Astron. Astrophys. 143, 421
Zickgraf, F.-J., Wolf, B., Stahl, O., Leitherer, C, Appenzeller, I.: 1986, Astron. Astrophys. 163, 119
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 Kluwer Academic Publishers
About this paper
Cite this paper
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
Download citation
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
eBook Packages: Springer Book Archive