The top documents tagged [continuum opacity]

NEGATIVE ION PLASMAS Professor Robert L. Merlino Department of Physics & Astronomy University of Iowa Plasma Physics Seminar, April 23, 2007
Documents NEGATIVE ION PLASMAS Professor Robert L. Merlino Department of Physics & Astronomy University of Iowa Plasma Physics Seminar, April 23, 2007

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Radiatively Driven Winds and Aspherical Mass Loss Stan Owocki U. of Delaware collaborators: Ken GayleyU. Iowa Nir Shaviv Hebrew U. Rich TownsendU. Delaware
Documents Radiatively Driven Winds and Aspherical Mass Loss Stan Owocki U. of Delaware collaborators: Ken GayleyU. Iowa Nir Shaviv Hebrew U. Rich TownsendU. Delaware

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Breaching the Eddington Limit in the Most Massive, Most Luminous Stars Stan Owocki Bartol Research Institute University of Delaware Collaborators: Nir
Documents Breaching the Eddington Limit in the Most Massive, Most Luminous Stars Stan Owocki Bartol Research Institute University of Delaware Collaborators: Nir

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X-ray Emission Line Profiles of Hot Stars David H. Cohen and Stanley P. Owocki Presented at “Two Years of Chandra Science” Washington, D.C., September
Documents X-ray Emission Line Profiles of Hot Stars David H. Cohen and Stanley P. Owocki Presented at “Two Years of Chandra Science” Washington, D.C., September

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Evolved Massive Stars. Wolf-Rayet Stars Classification WNL - weak H, strong He, NIII,IV WN2-9 - He, N III,IV,V earliest types have highest excitation
Documents Evolved Massive Stars. Wolf-Rayet Stars Classification WNL - weak H, strong He, NIII,IV WN2-9 - He, N III,IV,V earliest types have highest excitation

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Exoplanet Transit Spectroscopy February 7, 2014 Avi M. Mandell NASA GSFC Collaborators: Korey Haynes Evan Sinukoff Drake Deming Adam Burrows Nikku Madhusudhan
Documents Exoplanet Transit Spectroscopy February 7, 2014 Avi M. Mandell NASA GSFC Collaborators: Korey Haynes Evan Sinukoff Drake Deming Adam Burrows Nikku Madhusudhan

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New Model Atmospheres for Hydrogen-Deficient Stars May 3 rd, 2006 Natalie Behara Armagh Observatory
Documents New Model Atmospheres for Hydrogen-Deficient Stars May 3 rd, 2006 Natalie Behara Armagh Observatory

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Line Shapes in Hot Stars : Hydrodynamics & Wind Mass-Loss Rates
Documents Line Shapes in Hot Stars : Hydrodynamics & Wind Mass-Loss Rates

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NEGATIVE ION PLASMAS
Documents NEGATIVE ION PLASMAS

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Transit Spectroscopy w/ WFC3 March 11, 2014 Avi M. Mandell NASA GSFC Collaborators: Korey Haynes Evan Sinukoff Drake Deming Adam Burrows Nikku Madhusudhan
Documents Transit Spectroscopy w/ WFC3 March 11, 2014 Avi M. Mandell NASA GSFC Collaborators: Korey Haynes Evan Sinukoff Drake Deming Adam Burrows Nikku Madhusudhan

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Conclusions The prototype Pup (O4 I) has X-ray emission line profiles consistent with a simple spherically symmetric wind shock model. What can lead
Documents Conclusions The prototype Pup (O4 I) has X-ray emission line profiles consistent with a simple spherically symmetric wind shock model. What can lead

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NEGATIVE ION PLASMAS
Documents NEGATIVE ION PLASMAS

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