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- W3215696506 abstract "We have developed a new method for spectral analysis of binaries. Our method successfully identifies SB2 candidates from high-resolution Gaia-ESO spectra. Compared to the commonly used cross-correlation function analysis, it works for binaries with rapidly rotating components. We test our method on synthetic and observational spectra of BAFG-stars in the open cluster M 11. We confirm five previously detected SB2 candidates and find 19 new ones. For three SB2 candidates we find circular orbits and obtain dynamical mass ratios." @default.
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- W3215696506 date "2021-11-25" @default.
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- W3215696506 title "Double-lined spectroscopic binaries in M11" @default.
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- W3215696506 doi "https://doi.org/10.1093/mnras/stab3365" @default.
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