activity
20152025
most citedThe Magnetic Early B-type Stars I: Magnetometry and Rotation

101 citations · 753 across the 37 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

47 papers · 1 filter

astro-ph.SR2025

Discovery of the binary nature of the magnetospheric B-type star Oph A

M. E. Shultz, I. Berry, D. Bohlender +11

The nearby B-type star Oph A was recently identified as a rapidly rotating magnetic B-type star with variable radio and X-ray emission consistent with a magnetospheric origin.…

astro-ph.SR20243 cited

HD 34736: An intensely magnetised double-lined spectroscopic binary with rapidly-rotating chemically peculiar B-type components

E. Semenko, O. Kochukhov, Z. Mikulášek +21

We report the results of a comprehensive study of the spectroscopic binary (SB2) system HD 34736 hosting two chemically peculiar (CP) late B-type stars. Using new and archival obse…

astro-ph.SR20221 cited

Spin-down and reduced mass loss in early-type stars with large-scale magnetic fields

Z. Keszthelyi, A. de Koter, Y. Götberg +12

Magnetism can greatly impact the evolution of stars. In some stars with OBA spectral types there is direct evidence via the Zeeman effect for stable, large-scale magnetospheres, wh…

astro-ph.SR202228 cited

The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities

Z. Keszthelyi, A. de Koter, Y. Götberg +12

Magnetic fields can drastically change predictions of evolutionary models of massive stars via mass-loss quenching, magnetic braking, and efficient angular momentum transport, whic…

astro-ph.SR202216 cited

Testing a scaling relation between coherent radio emission and physical parameters of hot magnetic stars

Barnali Das, Poonam Chandra, Matt E. Shultz +4

Coherent radio emission via electron cyclotron maser emission (ECME) from hot magnetic stars was discovered more than two decades ago, but the physical conditions that make the gen…

astro-ph.SR202237 cited

Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars

Stanley P Owocki, Matt E. Shultz, Asif ud-Doula +3

Magnetic B-stars often exhibit circularly polarized radio emission thought to arise from gyrosynchrotron emission by energetic electrons trapped in the circumstellar magnetosphere.…