'Stellar winds' presentation slideshows

Stellar winds - PowerPoint PPT Presentation


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

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

By agalia
(152 views)

PRINCIPLES OF STELLAR STRUCTURE AND EVOLUTION

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

By yank
(178 views)

Protostars, nebulas and Brown dwarfs

Protostars, nebulas and Brown dwarfs

Protostars, nebulas and Brown dwarfs. Just before you meet with your black hole partner let’s talk a little more about protostars and star formation, use the following to enrich your posters on star formation.

By chipo
(146 views)

VLASS – Galactic Science

VLASS – Galactic Science

VLASS – Galactic Science. Life cycle of star f ormation in our Galaxy as a proxy for understanding the Local Universe legacy science. Infrared GLIMPSE survey. VLASS – Galactic Science. HST image of NGC 3603, showing a cluster of massive star formation.

By isolde
(165 views)

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

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.

By tyne
(157 views)

Leaky Stars:

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

By colin
(182 views)

Supernov æ as Cosmic-ray sources

Supernov æ as Cosmic-ray sources

Supernov æ as Cosmic-ray sources. II. Massive star formation regions & Superbubbles. A. Marcowith (L.P.T.A.). Outlines. OB association (OBa) and Super-bubbles (SB): a short overview. Massive stars clusters Supernov æ in Super-bubbles

By magar
(109 views)

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

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.

By nellie
(125 views)

Leaky Stars:

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

By lasley
(0 views)

Turbulence

Turbulence

Turbulence. 14 April 2003 Astronomy G9001 - Spring 2003 Prof. Mordecai-Mark Mac Low. General Thoughts. Turbulence often identified with incompressible turbulence only More general definition needed (V ázquez-Semadeni 1997) Large number of degrees of freedom

By dmetz
(3 views)


View Stellar winds PowerPoint (PPT) presentations online in SlideServe. SlideServe has a very huge collection of Stellar winds PowerPoint presentations. You can view or download Stellar winds presentations for your school assignment or business presentation. Browse for the presentations on every topic that you want.