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...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , , , |
|---|---|
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
IOP Publishing
2025-01-01
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| Cyfres: | The Astronomical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-3881/ada5f5 |
| Tagiau: |
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