Abstract
Speckle spectroscopy is a method to obtain objective spectra of stellar objects with high spatial resolution. We conducted speckle spectroscopic observations of binary stars at the Okayama Astrophysical Observatory in Japan and at the San Pedro Mártir Observatory in Mexico. Spectra of primary and secondary stars are spatially separated and the spectral distribution around Ha line is examined. We report observational results for some Be and B binary stars.
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Baba, N. et al. (1997). Observations of Be and B Binary Stars with the Speckle Spectroscopic Method. In: Docobo, J.A., Elipe, A., McAlister, H. (eds) Visual Double Stars: Formation, Dynamics and Evolutionary Tracks. Astrophysics and Space Science Library, vol 223. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1477-3_8
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DOI: https://doi.org/10.1007/978-94-009-1477-3_8
Publisher Name: Springer, Dordrecht
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