193. More on wide binaries

The origin of wide binary stars remains something of a mystery. In two earlier essays I looked at how Gaia detects them, and at suggestions that their orbits are inconsistent with Newtonian dynamics. Recent Gaia results throw new light on their formation, while researchers are still divided on the very long-period orbits.

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2024-09-09
DOI
https://doi.org/10.5281/zenodo.14599468
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00
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article

193. More on wide binaries

Zenodo (CERN European Organization for Nuclear Research)
Stellar, planetary, and galactic studies
article

193. More on wide binaries

article en

Abstract

The origin of wide binary stars remains something of a mystery. In two earlier essays I looked at how Gaia detects them, and at suggestions that their orbits are inconsistent with Newtonian dynamics. Recent Gaia results throw new light on their formation, while researchers are still divided on the very long-period orbits.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 64%
Stellar, planetary, and galactic studies
DOIOpen Access PDFOpenAlex
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193. More on wide binaries · Zenodo (CERN European Organization for Nuclear Research) (2024) | TGRS Research Map | TGRS