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- W104487442 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." @default.
- W104487442 created "2016-06-24" @default.
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- W104487442 date "1988-01-01" @default.
- W104487442 modified "2023-09-23" @default.
- W104487442 title "Highly resolved emission-line profiles of B[e] -supergiants" @default.
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- W104487442 doi "https://doi.org/10.1007/978-94-009-2941-8_18" @default.
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