Three-dimensional Orbit and Dynamical Masses of GJ 105 AC

The precision of stellar models is higher than the precision at which we are able to measure the masses of most stars, with the notable exception of binaries where we can determine dynamical masses of the component stars. In addition to well-measured stellar properties, the ideal benchmark star is f...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Cayla M. Dedrick, Jason T. Wright, Jason D. Eastman, Cullen H. Blake, Samson A. Johnson, Peter Plavchan, John Asher Johnson, David H. Sliski, Maurice L. Wilson, Robert A. Wittenmyer, Thomas Barclay, Jonathan Horner, Stephen R. Kane, Sharon X. Wang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Subjects:
Astrometric binary stars
Spectroscopic binary stars
Companion stars
Radial velocity
Astrometry
Stellar evolution
Online Access:https://doi.org/10.3847/1538-4357/adc564

Internet

https://doi.org/10.3847/1538-4357/adc564

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