The Likelihood of Hosting Undetected Brown Dwarfs in the Solar Vicinity
Diana Bakirova, Oleg Malkov

TL;DR
This paper estimates the probability of undetected brown dwarfs existing near the Sun, suggesting a significant chance of a nearby brown dwarf within 1.2 parsecs, and discusses why it remains undiscovered.
Contribution
It provides a new probabilistic model for the presence of undetected brown dwarfs in the solar neighborhood based on corrected observational data.
Findings
Approximately 50% chance of a brown dwarf within 1.2 parsecs
Discussion on possible multiplicity of the undetected object
Analysis of reasons for non-detection so far
Abstract
Based on the spatial distribution of objects in the solar neighbourhood with a radius of 20 parsecs, and after correcting for the incompleteness of observational data, an expression was obtained for estimating the probability of finding an object at a given distance from the Sun. According to these estimates, with a probability of about 0.5, there exists a brown dwarf in the immediate solar vicinity (< 1.2 pc). The possible multiplicity of this hypothetical object is discussed, as well as the reasons why it has not yet been detected.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · History and Developments in Astronomy · Radioactive Decay and Measurement Techniques
