Detection of 2460 double-lined spectroscopic binary candidates in the LAMOST-MRS using projected rotational velocities and a binary spectral model

Author:

Kovalev Mikhail1234ORCID,Chen Xuefei125,Han Zhanwen125ORCID

Affiliation:

1. Yunnan Observatories, Chinese Academy of Sciences , Kunming 650216, China

2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences , Kunming 650011, China

3. Sternberg Astronomical Institute , Leninskie Gory, Moscow 119992, Russia

4. Max Planck Institute for Astronomy , D-69117 Heidelberg, Germany

5. Center for Astronomical Mega-Science, Chinese Academy of Sciences , 20A Datun Road, Chaoyang District, Beijing 100012, China

Abstract

ABSTRACT We present a new method for the detection of double-lined spectroscopic binaries (SB2s) using Vsin i values from spectral fits. The method is tested on synthetic and real spectra from the Large Sky Area Multi-Object fiber Spectroscopic Telescope Medium Resolution Survey. It can reliably detect SB2 candidates for double-lined binaries with $V \sin {i}_1+V \sin {i}_2\lt 300\, {\rm km}\, {\rm s}^{-1}$ if the radial velocity separation is large enough. Using this method, we detected 2460 SB2 candidates, 1410 of which are new discoveries. We confirmed the correlation between the radial velocity separation estimated by the binary model and Vsin i0 estimated by the single-star model using the selected sample. Additionally, our method found one new SB2 candidate in open cluster M11.

Funder

National Key Research and Development Program of China

Natural Science Foundation of China

Chinese Academy of Sciences

National Development and Reform Commission

European Space Agency

ESO

CDS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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