2023A&A...671A..92C


Query : 2023A&A...671A..92C

2023A&A...671A..92C - Astronomy and Astrophysics, volume 671A, 92 (2023/3-1)

A spectroscopic modelling method for the detached eclipsing binaries to derive atmospheric parameters.

CHEN X.-L., LUO A.-L., CHEN J.-J., WANG R., ZHANG X.-B., HOU W., QIU B. and ZUO F.

Abstract (from CDS):

Based on luminosity contributions, we develop aspectroscopic modelling method to derive atmospheric parameters of component stars in binary systems. The method is designed for those spectra of binaries that show double-lined features due to radial-velocity differences between the component stars. We first derive the orbital parameters and the stellar radii by solving the light and radial-velocity curves. The luminosity contributions in different phases can then be calculated. We construct a synthesised double-lined spectra model by superposing theoretical single-star spectra according to the luminosity contributions. Finally, we derive the atmospheric parameters of each component star using the model-fitting method. For multi-epoch double-lined spectra observed by the Large sky Area Multi-Object Spectroscopic Telescope (LAMOST) Medium Resolution Survey (R ~ 7500), our method gives robust results for detached eclipsing binary systems observed in different orbital phases. Furthermore, this method can also be applied to other spectroscopic data with different resolutions as long as the systems are detached eclipsing binaries with nearly spherical stars.

Abstract Copyright: © The Authors 2023

Journal keyword(s): methods: data analysis - binaries: eclipsing - binaries: spectroscopic

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 HD 285001 EB* 05 02 10.1739163416 +22 25 23.888586432   12.04 10.98     K2 6 0
2 KOI-7013 EB* 19 29 11.2175040600 +44 16 49.949371668           F8V 23 0

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