Transit time derivation for hot planet bow-shocks
P. Wilson Cauley, Evgenya L. Shkolnik, and Joe Llama

TL;DR
This paper provides an analytical method to estimate transit times of hot planet bow-shocks, aiding observational planning of these phenomena.
Contribution
It introduces a new analytical approach for calculating hot planet bow-shock transit times, enhancing observational strategies.
Findings
Analytical estimates of bow-shock transit times provided
Method improves planning accuracy for observations
Applicable to hot planet systems
Abstract
We present an analytical estimate of hot planet bow-shock transit times that will be useful for planning observations of such signatures.
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