Difference between revisions of "Novel Method for the Evaluation of the Rotation Velocity of Solar-like Stars"
Jump to navigation
Jump to search
(Imported from text file) |
(Imported from text file) |
||
| Line 17: | Line 17: | ||
[[Category:Scientific Paper|novel method evaluation rotation velocity solar-like stars]] | [[Category:Scientific Paper|novel method evaluation rotation velocity solar-like stars]] | ||
| − | [[Category:Gravity]] | + | [[Category:Gravity|novel method evaluation rotation velocity solar-like stars]] |
| − | [[Category:Cosmology]] | + | [[Category:Cosmology|novel method evaluation rotation velocity solar-like stars]] |
Latest revision as of 19:45, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Novel Method for the Evaluation of the Rotation Velocity of Solar-like Stars |
| Read in full | Link to paper |
| Author(s) | Thierry De Mees |
| Keywords | Sun, solar-like stars, surface gravity, rotation velocity, gravitational constant |
| Published | 2012 |
| Journal | General Science Journal |
| No. of pages | 3 |
Read the full paper here
Abstract
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.
