'Stellar winds' presentation slideshows

1.06k views • 92 slides

Leaky Stars:

Leaky Stars:. Pulsations, Waves, and Turbulence in Stellar Winds across the H-R Diagram. Steven R. Cranmer & many others Harvard-Smithsonian Center for Astrophysics. Leaky Stars:. Outline: Background: history & basic physics The Sun: coronal heating & fast solar wind

823 views • 60 slides

Leaky Stars:

Leaky Stars:. Pulsations, Waves, and Turbulence in Stellar Winds across the H-R Diagram. Steven R. Cranmer & many others Harvard-Smithsonian Center for Astrophysics. Leaky Stars:. Outline: Background: history & basic physics The Sun: coronal heating & fast solar wind

606 views • 60 slides

Turbulence

377 views • 33 slides

Radio-loud AGN as sources for ultra-high-energy cosmic rays

Radio-loud AGN as sources for ultra-high-energy cosmic rays. Martin Hardcastle Hertfordshire SOCoR , Trondheim, 17 th June 2009

471 views • 28 slides

Protostars, nebulas and Brown dwarfs

372 views • 17 slides

Stephen St. Vincent (Swarthmore, class of 2007) Advisor: Prof. David Cohen

Visualizing Numerical Simulations of Magnetized Stellar Winds, and the Synthesis of Observational Diagnostics. Stephen St. Vincent (Swarthmore, class of 2007) Advisor: Prof. David Cohen.

268 views • 14 slides

Trends in the Chandra X-Ray Spectra of O and Early B Stars

Trends in the Chandra X-Ray Spectra of O and Early B Stars. June 24, 2008. Spectra of Stars. We know that spectra result from physical processes within stars. They often reflect physical properties of the stars that created them. ex. Optical Spectra. X-Ray Spectra of O and Early B Stars.

268 views • 10 slides

256 views • 8 slides

PRINCIPLES OF STELLAR STRUCTURE AND EVOLUTION

PRINCIPLES OF STELLAR STRUCTURE AND EVOLUTION. CESARE CHIOSI UNIVERSITY OF PADOVA, ITALY. The stars. Emit radiation Magnitudes, colors, spectra Emit matter Stellar winds, ISM enrichment Synthsize elements Generate the elemental species we know

227 views • 4 slides