Magnetic topology of low-mass stars : changes in coronal structure and emission measures across the fully convective boundary
M Dwarfs are becoming increasingly important in the investigation of magnetic fields. These low mass stars span a range of masses that coincide with a change in the internal structure from partly convective to fully convective. Despite this, these stars remain extremely magnetically active and exhib...
| Main Author: | |
|---|---|
| Other Authors: | |
| Published: |
University of St Andrews
2014
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.647803 |