Intermediate-mass mergers explain the disputed origin and B[e] properties of several FS CMa stars.
Refined Physical Properties of the HD327083 Binary System.Odessa Astron
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Synthetic spectra and MCMC analysis establish deuterium detection limits in early-type stars as a function of SNR, Teff, and v sin i, with upper limits D/H < -5.5 dex for HD 32115 and < -4.9 dex for 21 Peg.
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Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars
Intermediate-mass mergers explain the disputed origin and B[e] properties of several FS CMa stars.
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Detectability of deuterium in spectra of early-type stars
Synthetic spectra and MCMC analysis establish deuterium detection limits in early-type stars as a function of SNR, Teff, and v sin i, with upper limits D/H < -5.5 dex for HD 32115 and < -4.9 dex for 21 Peg.