activity
19952026
most citedDynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: I. Isothermal, Nonrotating, Radially Driven Flow

443 citations · 7.6k across the 140 of their papers we have counts for

collaborators

144 papers

astro-ph.HE2026

Wind-driven angular momentum removal and X-ray ionization effects in Roche-lobe overflowing HMXBs

Atsuo T. Okazaki, Stanley P. Owocki

We investigate the dynamical interaction between stellar winds and Roche-lobe overflow (RLO) streams in high-mass X-ray binaries using three-dimensional SPH simulations. We show th…

astro-ph.SR2026

Coherent and Incoherent Emission from the Ordered Magnetospheres of Low-Mass Stars, UCDs, and Massive Stars

Francesco Cavallaro, Paolo Leto, Barnali Das +15

Massive early-type (B/A) stars and ultracool dwarfs (UCDs) represent two distinct regimes in which ordered, large-scale magnetospheres are observed. In rapidly rotating massive sta…

astro-ph.SR2023

On the spatial distribution of electron energy loss due to gyro-cooling in hot-star magnetospheres

B. Das, S. P. Owocki

Hot magnetic stars often exhibit incoherent circularly polarized radio emission thought to arise from gyro-synchrotron emission by energetic electrons trapped in the circumstellar…

astro-ph.SR2023★ 9 cited

3D MHD models of the centrifugal magnetosphere from a massive star with an oblique dipole field

Asif ud-Doula, Stanley P. Owocki, Christopher Russell +2

We present results from new self-consistent 3D MHD simulations of the magnetospheres from massive stars with a dipole magnetic axis that has a non-zero obliquity angle () to the…

astro-ph.SR2022★ 2 cited

Magnetically confined wind shock

Asif ud-Doula, Stan Owocki

Many stars across all classes possess strong enough magnetic fields to influence dynamical flow of material off the stellar surface. For the case of massive stars (O and B types),…

astro-ph.SR2022★ 16 cited

Method and new tabulations for flux-weighted line-opacity and radiation line-force in supersonic media

L. G. Poniatowski, N. D. Kee, J. O. Sundqvist +7

In accelerating and supersonic media, the interaction of photons with spectral lines can be of ultimate importance. However, fully accounting for such line forces currently can onl…