activity
20022024
most citedThe surprising magnetic topology of tauSco: fossil remnant or dynamo output?

496 citations · 4.2k across the 63 of their papers we have counts for

collaborators

64 papers

astro-ph.SR2024

Epsilon Sagittarii: An Extreme Rapid Rotator with a Decretion Disk

Jeremy Bailey, Fiona Lewis, Ian D. Howarth +3

We report high-precision multi-wavelength linear-polarization observations of the bright B9 (or A0) star Sagittarii. The polarization shows the distinctive wavelength dependenc…

astro-ph.SR2024

Rapid polarization variations in the O4 supergiant Puppis

Jeremy Bailey, Ian D. Howarth, Daniel V. Cotton +5

We present time-series linear-polarization observations of the bright O4 supergiant Puppis. The star is found to show polarization variation on timescales of around an hour and…

astro-ph.SR2023★ 6 cited

Discovery of Dipolar Chromospheres in Two White Dwarfs

J. Farihi, J. J. Hermes, S. P. Littlefair +3

This paper reports the ULTRACAM discovery of dipolar surface spots in two cool magnetic white dwarfs with Balmer emission lines, while a third system exhibits a single spot, simila…

astro-ph.SR2023★ 7 cited

A study of the rapid rotator Aql: differential surface rotation?

Ian D. Howarth, Jeremy Bailey, Daniel V. Cotton +1

We report new, extremely precise, photopolarimetry of the rapidly-rotating A0 main-sequence star Aql, covering the wavelength range 400--900nm, which reveals a rotational…

astro-ph.SR2022★ 9 cited

A study of the F-giant star Scorpii A: a post-merger rapid rotator?

Fiona Lewis, Jeremy Bailey, Daniel V. Cotton +3

We report high-precision observations of the linear polarization of the F1III star Scorpii. The polarization has a wavelength dependence of the form expected for a rapid ro…

astro-ph.SR2022★ 16 cited

Properties of the Be-type stars in 30 Doradus

P. L. Dufton, D. J. Lennon, J. I. Villasenor +5

The evolutionary status of Be-type stars remains unclear, with both single-star and binary pathways having been proposed. Here, VFTS spectroscopy of 73 Be-type stars, in the spectr…