Corotating Interaction Regions and clumping

Corotating Interaction Regions and clumping

We present hydrodynamical models for Corotating Interaction Regions, which were used by Lobel (2007) to model the Discrete Absorption Components in HD 64760. We also discuss our failure to model the rotational modulations seen in the same star.

Bibliographic Details
Main Author:	Blomme, R.
Format:	Others
Language:	English
Published:	Universität Potsdam 2007
Subjects:	Astronomy and allied sciences
Online Access:	http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18100 http://opus.kobv.de/ubp/volltexte/2008/1810/

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