activity
20042026
most citedThe MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

232 citations · 955 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

Magnetically guided accretion and extremely slow rotation in a metal-enriched white dwarf

S. Bagnulo, M. A. Stroet, C. P. Folsom +3

White dwarfs that show atmospheric metal enrichment offer a direct window into the bulk composition of exoplanetary material and provide some of the most direct constraints on the…

astro-ph.SR2024★ 1 cited

Searching for magnetic fields in featureless white dwarfs with the DIPOL-UF polarimeter at the Nordic Optical Telescope

A. Berdyugin, J. D. Landstreet, S. Bagnulo +2

About 20% of the white dwarfs possess a magnetic field that may be detected by the splitting and/or polarization of their spectral lines. As they cool, the effective temperatures o…

astro-ph.SR2024★ 6 cited

Atmospheric heating and magnetism driven by Ne distillation in isolated white dwarfs

A. F. Lanza, N. Z. Rui, J. Farihi +2

The origin of atmospheric heating in the cool, magnetic white dwarf GD 356 remains unsolved nearly 40 years after its discovery. This once idiosyncratic star with $T_{\rm eff}\appr…

astro-ph.SR2024

Metal accretion scars may be common on magnetic, polluted white dwarfs

S. Bagnulo, J. D. Landstreet, J. Farihi +3

More than 30% of white dwarfs exhibit atmospheric metals, which are understood to be from recent or ongoing accretion of circumstellar debris. In cool white dwarfs, surface motions…

astro-ph.SR2022★ 8 cited

The magnetic field of the chemically peculiar star V352Peg

L. Fréour, C. Neiner, J. D. Landstreet +2

We present a spectropolarimetric analysis of the hot star V352Peg. We have acquired 18 spectropolarimetric observations of the star with ESPaDOnS at the CFHT between 2018 and 2019…

astro-ph.SR2022★ 65 cited

MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars

M. E. Shultz, S. P. Owocki, A. ud-Doula +13

Numerous magnetic hot stars exhibit gyrosynchrotron radio emission. The source electrons were previously thought to be accelerated to relativistic velocities in the current sheet f…