Hot subdwarf-B (sdB) stars in long-period binaries are found to be on eccentric orbits, even though current binary-evolution theory predicts that these objects are circularized before the onset of Roche lobe overflow (RLOF). To increase our understanding of binary interaction processes during the RLOF phase, we started a long-term observing campaign to study wide sdB binaries. In this paper, we present a sample of composite binary sdBs, and the results of the spectral analysis of nine such systems. The grid search in stellar parameters (GSSP) code is used to derive atmospheric parameters for the cool companions. To cross-check our results and also to characterize the hot subdwarfs, we used the independent XTGRID code, which employs TLUSTY non-local thermodynamic equilibrium models to derive atmospheric parameters for the sdB component and PHOENIX synthetic spectra for the cool companions. The independent GSSP and XTGRID codes are found to show good agreement for three test systems that have atmospheric parameters available in the literature. Based on the rotational velocity of the companions, we make an estimate for the mass accreted during the RLOF phase and the minimum duration of that phase. We find that the mass transfer to the companion is minimal during the subdwarf formation.
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2018 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Binaries: spectroscopic, Stars: abundances, Stars: fundamental parameters, Stars: horizontal branch, Stars: mass-loss, Subdwarfs
Vos, Joris, Péter Németh, Maja Vuc̆ković, Roy Østensen, and Steven Parsons. "Composite hot subdwarf binaries–I. The spectroscopically confirmed sdB sample." Monthly Notices of the Royal Astronomical Society 473, no. 1 (2018): 693-709.
Monthly Notices of the Royal Astronomical Society