His main research concerns Astrophysics, Stars, Astronomy, Stellar rotation and Line. Stanley P. Owocki studies Stellar mass which is a part of Astrophysics. His Stars research is multidisciplinary, incorporating elements of Gravitation, Gravitational potential and Rotation.
Stanley P. Owocki works mostly in the field of Stellar rotation, limiting it down to concerns involving Radius and, occasionally, Opacity. He has included themes like Acceleration and Supersonic speed in his Line study. His work carried out in the field of Radiative transfer brings together such families of science as Instability and Radial velocity.
Stanley P. Owocki mostly deals with Astrophysics, Stars, Astronomy, Radiative transfer and Line. His work deals with themes such as Spectral line, Emission spectrum and Instability, which intersect with Astrophysics. His Spectral line study combines topics in areas such as Light curve and Absorption.
As part of one scientific family, Stanley P. Owocki deals mainly with the area of Stars, narrowing it down to issues related to the Magnetic field, and often Dipole. His research investigates the connection with Radiative transfer and areas like Computational physics which intersect with concerns in Classical mechanics. His studies deal with areas such as Supergiant, Photosphere and Stellar wind as well as Line.
Stanley P. Owocki mainly focuses on Astrophysics, Stars, Radiative transfer, Astronomy and Magnetic field. His Astrophysics research is multidisciplinary, relying on both Spectral line, X-ray and Magnetosphere. His study in Stars is interdisciplinary in nature, drawing from both Instability, Magnetohydrodynamics, Plasma and Opacity.
His Radiative transfer study incorporates themes from Luminosity and Computational physics. His Magnetic field study which covers Dipole that intersects with OB star. His work focuses on many connections between Line and other disciplines, such as Photosphere, that overlap with his field of interest in Radiation.
His scientific interests lie mostly in Astrophysics, Stars, O-type star, Astronomy and Magnetic field. The Astrophysics study combines topics in areas such as Magnetohydrodynamics, Opacity, Spectral line, Radiative transfer and Magnetosphere. His Radiative transfer study integrates concerns from other disciplines, such as Shock wave, Distribution function and Instability.
The study incorporates disciplines such as Line, Gravitation, Radius and Kinetic energy in addition to Stars. Stanley P. Owocki has researched Line in several fields, including Supergiant, Photosphere and Absorption. His O-type star research focuses on Plasma and how it connects with Shock.
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Time-dependent models of radiatively driven stellar winds. I - Nonlinear evolution of instabilities for a pure absorption model
Stanley P. Owocki;John I. Castor;George B. Rybicki.
The Astrophysical Journal (1988)
On the role of continuum-driven eruptions in the evolution of very massive stars and Population III stars
Nathan Smith;Stanley P. Owocki.
The Astrophysical Journal (2006)
Dynamical Simulations of Magnetically Channeled Line-driven Stellar Winds. I. Isothermal, Nonrotating, Radially Driven Flow
Asif ud-Doula;Stanley P. Owocki.
The Astrophysical Journal (2002)
Be-star rotation: how close to critical?
Richard H.D. Townsend;Richard H.D. Townsend;Stanley P. Owocki;Stanley P. Owocki;Ian D. Howarth.
Monthly Notices of the Royal Astronomical Society (2004)
Hydrodynamical Simulations of Corotating Interaction Regions and Discrete Absorption Components in Rotating O-Star Winds
Steven R. Cranmer;Stanley P. Owocki.
The Astrophysical Journal (1996)
Instabilities in line-driven stellar winds. I - Dependence on perturbation wavelength
S. P. Owocki;G. B. Rybicki.
The Astrophysical Journal (1984)
Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: III. Angular Momentum Loss and Rotational Spindown
Asif ud-Doula;Stanley P. Owocki;Richard H.D. Townsend.
arXiv: Astrophysics (2008)
Inhibition of Wind-Compressed Disk Formation by Nonradial Line Forces in Rotating Hot-Star Winds
S. P. Owocki;S. R. Cranmer;K. G. Gayley.
The Astrophysical Journal (1996)
Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: II. The Effects of Field-Aligned Rotation
Asif ud-Doula;Stanley Owocki;Richard Townsend.
arXiv: Astrophysics (2007)
Chandra HETGS Multi-Phase Spectroscopy of the Young Magnetic O Star theta^1 Orionis C
Marc Gagne;Mary E. Oksala;David H. Cohen;Stephanie K. Tonnesen.
arXiv: Astrophysics (2005)
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