58 citations · 114 across the 16 of their papers we have counts for
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astro-ph.SR2021
Detecting the Zeeman effect in Massive Star Magnetospheres in the UV
C. Erba, V. Petit, K. Gayley +3
Approximately 7% of massive stars host stable surface magnetic fields that are strong enough to alter stellar evolution through their effect on the stellar wind. It is therefore cr…
astro-ph.SR2021★ 16 cited
Ultraviolet Line Profiles of Slowly Rotating Massive Star Winds Using the "Analytic Dynamical Magnetosphere" Formalism
C. Erba, A. David-Uraz, V. Petit +6
Recent large-scale spectropolarimetric surveys have established that a small but significant percentage of massive stars host stable, surface dipolar magnetic fields with strengths…
astro-ph.SR2021★ 9 cited
Confirmation of xi^1 CMa's ultra-slow rotation: magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines
C. Erba, M. E. Shultz, V. Petit +5
The magnetic beta Cep pulsator xi^1 CMa has the longest rotational period of any known magnetic B-type star. It is also the only magnetic B-type star with magnetospheric emission t…