Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems

We obtained new spectra of Kepler-34 and Kepler-35 with Keck-HIRES—nearly a decade after these systems were originally characterized with this spectrograph and other instruments—to search for radial velocity (RV) trends from a potential third stellar-mass companion at long periods. For Kepler-34, we...

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Main Authors: Carlos Jurado, Lauren M. Weiss, Laura Daclison, Benjamin M. Tofflemire, Jerome A. Orosz, William F. Welsh
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
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Online Access:https://doi.org/10.3847/1538-3881/ada5f5
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_version_ 1825206477827080192
author Carlos Jurado
Lauren M. Weiss
Laura Daclison
Benjamin M. Tofflemire
Jerome A. Orosz
William F. Welsh
author_facet Carlos Jurado
Lauren M. Weiss
Laura Daclison
Benjamin M. Tofflemire
Jerome A. Orosz
William F. Welsh
author_sort Carlos Jurado
collection DOAJ
description We obtained new spectra of Kepler-34 and Kepler-35 with Keck-HIRES—nearly a decade after these systems were originally characterized with this spectrograph and other instruments—to search for radial velocity (RV) trends from a potential third stellar-mass companion at long periods. For Kepler-34, we rule out coplanar stellar masses as low as 0.12 M _⊙ at an orbital period of  ≲52 yr. For Kepler-35, we rule out stellar masses of 0.13 M _⊙ at orbital periods of  ≲55 yr. Highly stable, extreme precision RV instruments, as well as improved methodologies in characterizing double-lined spectroscopic binaries that come with these new instruments, will provide an opportunity to push these mass limits lower in the future.
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spelling doaj-art-5aaa5017dbdc47489fb9e4104df3dd6c2025-02-07T08:38:10ZengIOP PublishingThe Astronomical Journal1538-38812025-01-01169312710.3847/1538-3881/ada5f5Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 SystemsCarlos Jurado0https://orcid.org/0009-0009-7568-8851Lauren M. Weiss1https://orcid.org/0000-0002-3725-3058Laura Daclison2Benjamin M. Tofflemire3https://orcid.org/0000-0003-2053-0749Jerome A. Orosz4https://orcid.org/0000-0001-9647-2886William F. Welsh5https://orcid.org/0000-0003-2381-5301Department of Physics and Astronomy, University of California , Los Angeles, CA 90095, USA ; carx207@g.ucla.edu; Department of Physics and Astronomy, University of Notre Dame , Notre Dame, IN 46556, USADepartment of Physics and Astronomy, University of Notre Dame , Notre Dame, IN 46556, USAInstitute for Astronomy, University of Hawaii at Manoa , Honolulu, HI 96822, USADepartment of Astronomy, The University of Texas at Austin , Austin, TX 78712, USADepartment of Astronomy, San Diego State University , San Diego, CA 92182, USADepartment of Astronomy, San Diego State University , San Diego, CA 92182, USAWe obtained new spectra of Kepler-34 and Kepler-35 with Keck-HIRES—nearly a decade after these systems were originally characterized with this spectrograph and other instruments—to search for radial velocity (RV) trends from a potential third stellar-mass companion at long periods. For Kepler-34, we rule out coplanar stellar masses as low as 0.12 M _⊙ at an orbital period of  ≲52 yr. For Kepler-35, we rule out stellar masses of 0.13 M _⊙ at orbital periods of  ≲55 yr. Highly stable, extreme precision RV instruments, as well as improved methodologies in characterizing double-lined spectroscopic binaries that come with these new instruments, will provide an opportunity to push these mass limits lower in the future.https://doi.org/10.3847/1538-3881/ada5f5Radial velocityEclipsing binary stars
spellingShingle Carlos Jurado
Lauren M. Weiss
Laura Daclison
Benjamin M. Tofflemire
Jerome A. Orosz
William F. Welsh
Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
The Astronomical Journal
Radial velocity
Eclipsing binary stars
title Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
title_full Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
title_fullStr Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
title_full_unstemmed Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
title_short Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
title_sort upper limits on stellar companions to the kepler 34 and kepler 35 systems
topic Radial velocity
Eclipsing binary stars
url https://doi.org/10.3847/1538-3881/ada5f5
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