Astrophysics

   

Novel Method for the Evaluation of the Rotation Velocity of Solar-like Stars

Authors: Thierry De Mees

The evaluation of stars’ properties is classically performed by comparing the stars’ light spectra and fluxes to the known solar properties. Another method to find the stars’ rotation velocity will be discussed here: the extrapolation to the other solar-like stars of an empiric solar property, which consists of a direct relationship between the star’s frequency and its surface gravity, without the need of any other parameters.

Comments: 3 Pages.

Download: PDF

Submission history

[v1] 2017-02-17 03:50:57

Unique-IP document downloads: 5 times

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus