• English
    • Norsk
  • English 
    • English
    • Norsk
  • Administration
View Item 
  •   Home
  • Øvrige samlinger
  • Høstingsarkiver
  • CRIStin høstingsarkiv
  • View Item
  •   Home
  • Øvrige samlinger
  • Høstingsarkiver
  • CRIStin høstingsarkiv
  • View Item
JavaScript is disabled for your browser. Some features of this site may not work without it.

Impact of magnetic fields on the structure of convective atmospheres of red giant stars

Klevas, J.; Kučinskas, A.; Wedemeyer, Sven; Ludwig, H.-G.
Journal article; PublishedVersion; Peer reviewed
View/Open
pp280-281.pdf (607.7Kb)
Year
2018
Permanent link
http://urn.nb.no/URN:NBN:no-68635

CRIStin
1649654

Metadata
Show metadata
Appears in the following Collection
  • Det matematisk-naturvitenskapelige fakultet [338]
  • Institutt for teoretisk astrofysikk [724]
  • CRIStin høstingsarkiv [16985]
Original version
Contributions of the Astronomical Observatory Skalnate Pleso. 2018, 48 (1), 280-281
Abstract
We use 3D magnetohydrodynamic CO5BOLD model atmospheres to study the interplay between magnetic fields and convection in the atmospheres of red giant stars. We find that vortex-like structures occur prominently in stars with stronger magnetic fields and lead to alterations of their thermal structures.
 
Responsible for this website 
University of Oslo Library


Contact Us 
duo-hjelp@ub.uio.no


Privacy policy
 

 

For students / employeesSubmit master thesisAccess to restricted material

Browse

All of DUOCommunities & CollectionsBy Issue DateAuthorsTitlesThis CollectionBy Issue DateAuthorsTitles

For library staff

Login
RSS Feeds
 
Responsible for this website 
University of Oslo Library


Contact Us 
duo-hjelp@ub.uio.no


Privacy policy