THE Hα EMISSION OF NEARBY M DWARFS AND ITS RELATION TO STELLAR ROTATION

The high-energy emission from low-mass stars is mediated by the magnetic dynamo. Although the mechanisms by which fully convective stars generate large-scale magnetic fields are not well understood, it is clear that, as for solar-type stars, stellar rotation plays a pivotal role. We present 270 new...

Full description

Bibliographic Details
Main Authors: Irwin, Jonathan (Author), Charbonneau, David (Author), Berlind, Perry (Author), Calkins, Michael L. (Author), Mink, Jessica (Author), Newton, Elisabeth R (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-06-08T13:59:53Z.
Subjects:
Online Access:Get fulltext

Similar Items