English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We report on attempts to measure the magnetic field of the pulsating B star$\nu$ Eridani with the Musicos spectropolarimeter attached to the 2m telescopeat the Pic du Midi, France. This object is one of the most extensively studiedstars for pulsation modes, and the existence of a magnetic field was suggestedfrom the inequality of the frequency separations of a triplet in the stars'oscillation spectrum. We show that the inferred 5-10 kG field was not presentduring our observations, which cover about one year. We discuss the influenceof the strong pulsations on the analysis of the magnetic field strength and setan upper limit to the effective longitudinal field strength and to the fieldstrength for a dipolar configuration. We also find that the observed wind linevariability is caused by the pulsations.Comment: 8 pages, 7 figures, accepted by A&

Attempts to measure the magnetic field of the pulsating B starνEridani