Conference paper Open Access

Stellar-Planet Interaction: Accretion from planetary wind

Colombo, Salvatore; Pillitteri, Ignazio; Orlando, Salvatore; Micela, Giuseppina

Hot Jupiters are perfect laboratories to study the processes of stellar-planet interaction. Due to their mass and proximity to the central star, the atmospheres of hot Jupiters are heated by the stellar radiation and, in some cases, they photoevaporate. The stellar wind is the medium where the planetary outflow expands. In this work, we model the interaction of the planetary wind with the star extended corona. We aim to understand whether this interaction may result in an enhanced stellar activity. 

Files (6.7 MB)
Name Size
Poster_cool_star20.5_Colombo.pdf
md5:92535fc562392c4b217b7ad59821d978 		6.7 MB Download
100
85
views
downloads
All versions This version
Views 100100
Downloads 8585
Data volume 565.8 MB565.8 MB
Unique views 100100
Unique downloads 8181
More info on how stats are collected.
Indexed in
Publication date:
February 25, 2021
DOI:
10.5281/zenodo.4562963

Zenodo DOI Badge

DOI 

10.5281/zenodo.4562963

Markdown 

[![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.4562963.svg)](https://doi.org/10.5281/zenodo.4562963)

reStructedText 

.. image:: https://zenodo.org/badge/DOI/10.5281/zenodo.4562963.svg
   :target: https://doi.org/10.5281/zenodo.4562963

HTML 

<a href="https://doi.org/10.5281/zenodo.4562963"><img src="https://zenodo.org/badge/DOI/10.5281/zenodo.4562963.svg" alt="DOI"></a>

Image URL 

https://zenodo.org/badge/DOI/10.5281/zenodo.4562963.svg

Target URL 

https://doi.org/10.5281/zenodo.4562963

Keyword(s):
Stellar-Planet Interaction exoplanet Star
Communities:
License (for files):
Creative Commons Attribution 4.0 International

Versions

Version 1 10.5281/zenodo.4562963 Feb 25, 2021
Cite all versions? You can cite all versions by using the DOI 10.5281/zenodo.4562962. This DOI represents all versions, and will always resolve to the latest one. Read more.

Share

Cite as

Export