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...
Saved in:
Main Authors: | , , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astronomical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-3881/ada5f5 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
_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. |
format | Article |
id | doaj-art-5aaa5017dbdc47489fb9e4104df3dd6c |
institution | Kabale University |
issn | 1538-3881 |
language | English |
publishDate | 2025-01-01 |
publisher | IOP Publishing |
record_format | Article |
series | The Astronomical Journal |
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 |
work_keys_str_mv | AT carlosjurado upperlimitsonstellarcompanionstothekepler34andkepler35systems AT laurenmweiss upperlimitsonstellarcompanionstothekepler34andkepler35systems AT lauradaclison upperlimitsonstellarcompanionstothekepler34andkepler35systems AT benjaminmtofflemire upperlimitsonstellarcompanionstothekepler34andkepler35systems AT jeromeaorosz upperlimitsonstellarcompanionstothekepler34andkepler35systems AT williamfwelsh upperlimitsonstellarcompanionstothekepler34andkepler35systems |