Corotating Interaction Regions and clumping

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dc.creatorBlomme, R.
dc.date2007-09-04
dc.date.accessioned2026-07-07T08:27:33Z
dc.date.available2026-07-07T08:27:33Z
dc.descriptionWe 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.
dc.description3 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0709.0489
dc.identifierhttp://arxiv.org/abs/0709.0489
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/137307
dc.subjectAstrophysics
dc.titleCorotating Interaction Regions and clumping
dc.typetext

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