The Internal Structure of M Dwarf Stars
Copyright policy ) Keisuke Kaminisi;
The Internal Structure of M Dwarf Stars
Abstract Models for M dwarfs which consist of a convective envelope and a radiative core are computed with the effects of electron degeneracy taken into account. The results show that in the middle M dwarf, such as Krüger 60A, O2 Eri C and Krüger 60B, the convective envelope extends inward attaining to more than 40% of the stellar radius and the degree of degeneracy at their centres ϕ0, reaches to nearly 0.00.
- Kumamoto University Japan
selected citations These citations are derived from selected sources.This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).0 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Average influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Average impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Average
selected citations
Citations provided by BIP!
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 0
Average
Average
Average
This action will publish the selected files and record in Zenodo. Are you sure you want to proceed?