Radial Velocity and Astrometric Evidence for a Close Companion to Betelgeuse
Morgan MacLeod, Sarah Blunt, Robert J. De Rosa, Andrea K. Dupree,, Thomas Granzer, Graham M. Harper, Caroline D. Huang, Emily M. Leiner, Abraham, Loeb, Eric L. Nielsen, Klaus G. Strassmeier, Jason J. Wang, Michael Weber

TL;DR
This study presents evidence suggesting Betelgeuse has a low-mass, nearly hidden companion star in a close orbit, which influences its observed variability and rapid rotation, indicating a binary system.
Contribution
It provides the first combined radial velocity and astrometric evidence for a close, low-mass companion to Betelgeuse, explaining its spin and variability.
Findings
Betelgeuse likely has a low-mass companion less than a solar mass.
The companion orbits at a 2,110-day period just over twice Betelgeuse's radius.
Future orbit decay will lead to the companion being swallowed within 10,000 years.
Abstract
We examine a century of radial velocity, visual magnitude, and astrometric observations of the nearest red supergiant, Betelgeuse, in order to reexamine the century-old assertion that Betelgeuse might be a spectroscopic binary. These data reveal Betelgeuse varying stochastically over years and decades due to its boiling, convective envelope, periodically with a ~yr long secondary period, and quasi-periodically from pulsations with periods of several hundred days. We show that the long secondary period is consistent between astrometric and RV datasets, and argue that it indicates a low-mass companion to Betelgeuse, less than a solar mass, orbiting in a 2,110 day period at a separation of just over twice Betelgeuse's radius. The companion star would be nearly twenty times less massive and a million times fainter than Betelgeuse, with similar effective temperature, effectively…
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Taxonomy
TopicsHistory and Developments in Astronomy · Gamma-ray bursts and supernovae · Stellar, planetary, and galactic studies
