No magnetic field variations with pulsation phase in the classical Cepheid star eta Aquilae

Details No magnetic field variations with pulsation phase in the classical Cepheid star eta Aquilae No magnetic field variations with pulsation phase in the classical Cepheid star eta Aquilae

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...392l..17w&link_type=abstract

Astronomy and Astrophysics, v.392, p.L17-L20 (2002)

Astronomy and Astrophysics

Astrophysics

11

Stars: Atmospheres, Stars: Variable: Delta Cep, Stars: Individual: Eta Aql, Stars: Magnetic Fields, Polarisation

Scientific paper

We report new high resolution Stokes V spectropolarimetry and ultra-high precision longitudinal magnetic field measurements of the pulsating classical Cepheid eta Aql which fail to corroborate the report by Plachinda (\cite{Plachinda}) of a ~ 100 G magnetic field in this star. Based on observations obtained using the MuSiCoS spectropolarimeter at Pic du Midi observatory.

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