Gas dynamic simulation of the star-planet interaction using a binary star model
D. E. Ionov, D. V. Bisikalo, P. V. Kaygorodov, V. I. Shematovich
TL;DR
This paper presents gas dynamic simulations of star-planet interactions, modeling the gaseous flow in the HD 209458 system to explain observational data from the HST, using a binary star simulation code.
Contribution
It introduces a novel application of binary star simulation code to model star-planet interactions, providing insights into the gas flow structure around hot Jupiters.
Findings
Model successfully reproduces observed gas flow patterns.
Simulation explains features observed with HST COS instrument.
Provides a framework for studying star-planet gas interactions.
Abstract
We have performed numerical simulations of the interaction between "hot Jupiter" planet and gas of the stellar wind using numerical code developed for investigations of binary stars. With this code we have modeled the structure of the gaseous flow in the system HD 209458. The results have been used to explain observations of this system performed with the COS instrument on-board the HST.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.