Stellar Flares and Coronal Structure

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

Coronal structure and coronal heating are intimately related in magnetically active stars. Coronal structure is commonly inferred from radio interferometry and from eclipse and rotational modulation studies. We discuss to what extent flares may be responsible for coronal structure and global observable properties in magnetically active stars.
to appear in proceedings of IAU Symposium 219, Stars as Suns: Activity, Evolution, Planets; preprint also at http://www.astro.phys.ethz.ch/papers/guedel/guedel_p_nf.html

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/7142

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0312378
 http://arxiv.org/abs/astro-ph/0312378

Collections

arXiv