S. P. Owocki

University of Delaware — United States

Physics and Astronomy · Physical Sciences

60h-index10.3kcitations504works0.52yr avg
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Research Topics

Stellar, planetary, and galactic studies(300), Astrophysics and Star Formation Studies(234), Astro and Planetary Science(121), Solar and Space Plasma Dynamics(112), Astrophysical Phenomena and Observations(90)

Publications503 total

A generalized semi-analytic model for the combined outflow from a cluster of stars with strong stellar winds
Monthly Notices of the Royal Astronomical Society·2025Open Access
Efficiency of viscous angular momentum transport in dissipating Be binaries
Astrophysics and Space Science·2025· 1 cited
Wind and Eruptive Mass Loss near the Eddington Limit
Galaxies·2025Open Access
Fundamentals of Astrophysics
Cambridge University Press eBooks·2025
A generalized semi-analytic model for the combined outflow from a cluster of stars with strong stellar winds
arXiv (Cornell University)·2025Open Access
Discovery of the binary nature of the magnetospheric B-type star <i>ρ</i> Oph A
Astronomy and Astrophysics·2025· 2 citedOpen Access
The effect of collisional cooling of energetic electrons on radio emission from the centrifugal magnetospheres of magnetic hot stars
Publications of the Astronomical Society of Australia·2025· 1 citedOpen Access
Magnetically Confined Wind Shock
2024
On the spatial distribution of electron energy loss due to gyro-cooling in hot star magnetospheres
Monthly Notices of the Royal Astronomical Society·2023Open Access
MOBSTER – VII. Using light curves to infer magnetic and rotational properties of stars with centrifugal magnetospheres
Monthly Notices of the Royal Astronomical Society·2023· 2 cited
MOBSTER -- VII. Using light curves to infer magnetic and rotational properties of stars with centrifugal magnetospheres
arXiv (Cornell University)·2023Open Access
3D MHD models of the centrifugal magnetosphere from a massive star with an oblique dipole field
Monthly Notices of the Royal Astronomical Society·2023· 8 citedOpen Access
3D MHD models of the centrifugal magnetosphere from a massive star with an oblique dipole field
arXiv (Cornell University)·2023Open Access
Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain
Astrophysics and Space Science·2022· 4 citedOpen Access
Winds and magnetospheres of stars and planets: similarities and differences
arXiv (Cornell University)·2022Open Access
Magnetically Confined Wind Shock
2022· 2 cited
Magnetically confined wind shock
arXiv (Cornell University)·2022Open Access
Discovery and origin of the radio emission from the multiple stellar system KQ Vel
Monthly Notices of the Royal Astronomical Society·2022· 4 cited
Obliquely Rotating Massive Star Magnetospheres
Proceedings of the International Astronomical Union·2022Open Access
Method and new tabulations for flux-weighted line-opacity and radiation line-force in supersonic media: Tables
Zenodo (CERN European Organization for Nuclear Research)·2022Open Access
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Frequent Co-authors

R. H. D. Townsend(12), Asif ud‐Doula(11), David H. Cohen(10), Steven R. Cranmer(7), J. O. Sundqvist(6), G. A. Wade(5), V. Pétit(4), Atsuo T. Okazaki(4), J. Puls(4), G. B. Rybicki(3), K. G. Gayley(3), M. E. Oksala(3), Jiřı́ Krtička(3), Christopher M. P. Russell(3), Marc Gagné(2), D. Bohlender(2), Th. Rivinius(2), E. Alécian(2), J. J. MacFarlane(2), G. Gräfener(2)