The null result of a search for pulsational variations of the surface magnetic field in the roAp star gamma Equulei

Details The null result of a search for pulsational variations of the surface magnetic field in the roAp star gamma Equulei The null result of a search for pulsational variations of the surface magnetic field in the roAp star gamma Equulei

2004-04-27

arxiv.org/abs/astro-ph/0404528v1

Mon.Not.Roy.Astron.Soc. 351 (2004) L34

Astronomy and Astrophysics

Astrophysics

Accepted by MNRAS

Scientific paper

10.1111/j.1365-2966.2004.07946.x

We describe an analysis of the time-resolved measurements of the surface magnetic field in the roAp star gamma Equ. We have obtained a high-resolution and high S/N spectroscopic time-series, and the magnetic field was determined using Zeeman resolved profiles of the Fe II 6149.25 A and Fe I 6173.34 A lines. Contrary to recent reports we do not find any evidence of magnetic variability with pulsation phase, and derive an upper limit of 5-10 G for pulsational modulation of the surface magnetic field in gamma Equ.

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