Corotating Interaction Regions and clumping

Details Corotating Interaction Regions and clumping Corotating Interaction Regions and clumping

2007-09-04

arxiv.org/abs/0709.0489v1

Astronomy and Astrophysics

Astrophysics

3 pages, 3 figures

Scientific paper

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.

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