activity
20042025
most citedAn unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova

94 citations · 636 across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.IM2025

Expanding stellar horizons with polarized light

J. Vandersnickt, R. Ochoa Armenta, V. Vanlaer +16

The polarization of light is a critically under-utilized, rich source of information in astronomy. For stars in particular, surface magnetism polarization that can be detected and…

astro-ph.SR2023★ 1 cited

TESS Cycle 2 observations of roAp stars with 2-min cadence data

D. L. Holdsworth, M. S. Cunha, M. Lares-Martiz +46

We present the results of a systematic search of the Transiting Exoplanet Survey Satellite (TESS) 2-min cadence data for new rapidly oscillating Ap (roAp) stars observed during the…

astro-ph.SR2022★ 5 cited

HD 213258: a new rapidly oscillating, super-slowly rotating, strongly magnetic Ap star in a spectroscopic binary

Gautier Mathys, Viktor Khalack, Oleksandr Kobzar +2

We report about HD 213258, an Ap star that we recently identified as presenting a unique combination of rare, remarkable properties. Our study of this star is based on ESPaDOnS Sto…

astro-ph.SR2022★ 7 cited

Analysis of eight magnetic chemically peculiar stars with rotational modulation

O. Kobzar, V. Khalack, D. Bohlender +9

Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar photometry to the astronomical community. We have used TESS data to study rotational mo…

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…

astro-ph.SR2021★ 56 cited

TESS survey of rotational and pulsational variability of mercury-manganese stars

O. Kochukhov, V. Khalack, O. Kobzar +4

Mercury-manganese (HgMn) stars are late-B upper main sequence chemically peculiar stars distinguished by large overabundances of heavy elements, slow rotation, and frequent members…