Stanley Owocki
Stanley Owocki
Professor of Astrophysics, University of Delaware
Verified email at - Homepage
Cited by
Cited by
Time-dependent models of radiatively driven stellar winds. I-Nonlinear evolution of instabilities for a pure absorption model
SP Owocki, JI Castor, GB Rybicki
The Astrophysical Journal 335, 914-930, 1988
On the role of continuum-driven eruptions in the evolution of very massive stars and population III stars
N Smith, SP Owocki
The Astrophysical Journal Letters 645 (1), L45, 2006
Hydrodynamical simulations of corotating interaction regions and discrete absorption components in rotating O-star winds
SR Cranmer, SP Owocki
arXiv preprint astro-ph/9508004, 1995
Be‐star rotation: how close to critical?
RHD Townsend, SP Owocki, ID Howarth
Monthly Notices of the Royal Astronomical Society 350 (1), 189-195, 2004
Instabilities in line-driven stellar winds. I-Dependence on perturbation wavelength
SP Owocki, GB Rybicki
The Astrophysical Journal 284, 337-350, 1984
Inhibition of wind-compressed disk formation by nonradial line forces in rotating hot-star winds
SP Owocki, SR Cranmer, KG Gayley
The Astrophysical Journal Letters 472 (2), L115, 1996
Dynamical simulations of magnetically channeled line-driven stellar winds. I. Isothermal, nonrotating, radially driven flow
SP Owocki
The Astrophysical Journal 576 (1), 413, 2002
A porosity-length formalism for photon-tiring-limited mass loss from stars above the Eddington limit
SP Owocki, KG Gayley, NJ Shaviv
The Astrophysical Journal 616 (1), 525, 2004
A rigidly rotating magnetosphere model for circumstellar emission from magnetic OB stars
RHD Townsend, SP Owocki
Monthly Notices of the Royal Astronomical Society 357 (1), 251-264, 2005
The outer evolution of instability-generated structure in radiatively driven stellar winds
MC Runacres, SP Owocki
Astronomy & Astrophysics 381 (3), 1015-1025, 2002
Sudden radiative braking in colliding hot-star winds
KG Gayley, SP Owocki, SR Cranmer
The Astrophysical Journal 475 (2), 786, 1997
Two-dimensional hydrodynamical simulations of wind-compressed disks around rapidly rotating B stars
SP Owocki, SR Cranmer, JM Blondin
The Astrophysical Journal 424, 887-904, 1994
A. ud-Doula, MiMeS Collaboration, A magnetic confinement versus rotation classification of massive-star magnetospheres
V Petit, SP Owocki, GA Wade, DH Cohen, JO Sundqvist, M Gagné, ...
MNRAS 429, 398-422, 2013
The MiMeS survey of magnetism in massive stars: introduction and overview
GA Wade, C Neiner, E Alecian, JH Grunhut, V Petit, B Batz, DA Bohlender, ...
Monthly Notices of the Royal Astronomical Society 456 (1), 2-22, 2016
Chandra HETGS multiphase spectroscopy of the young magnetic O star θ1 Orionis C
M Gagné, ME Oksala, DH Cohen, SK Tonnesen, SP Owocki, ...
The Astrophysical Journal 628 (2), 986, 2005
Accretion vs. colliding wind models for the gamma-ray binary LS I+ 61 303: an assessment
GE Romero, AT Okazaki, M Orellana, SP Owocki
Astronomy & Astrophysics 474 (1), 15-22, 2007
The effect of porosity on X-ray emission-line profiles from hot-star winds
SP Owocki, DH Cohen
The Astrophysical Journal 648 (1), 565, 2006
Dynamical simulations of magnetically channelled line-driven stellar winds–II. The effects of field-aligned rotation
A Ud-Doula, SP Owocki, RHD Townsend
Monthly Notices of the Royal Astronomical Society 385 (1), 97-108, 2008
Line-driven Stellar winds: the dynamical role of diffuse radiation gradients and limitations to the Sobolev approach
SP Owocki, J Puls
The Astrophysical Journal 510 (1), 355, 1999
Stellar envelope inflation near the Eddington limit-Implications for the radii of Wolf-Rayet stars and luminous blue variables
G Gräfener, SP Owocki, JS Vink
Astronomy & Astrophysics 538, A40, 2012
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