'Nucleosynthesis' presentation slideshows

Nucleosynthesis - PowerPoint PPT Presentation

Chapter 14

Chapter 14

Chapter 14. Cosmology. Cosmology . Cosmology , the study of the universe as a whole, can tell you where your matter came from and where it is going.

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716 views • 47 slides
Th e Bi g Bang

Th e Bi g Bang

Th e Bi g Bang. D r . Mike MacCallum Long Beach City College mmaccallu m @lbcc.edu. Astrono m y Pictur e o f th e D a y. http://apod.na s a.gov/apod/. ?. Astronome r o f th e W eek. Alan H. Guth. ?.

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516 views • 40 slides
HR Diagram for nearby stars atlasoftheuniverse/hr.html

HR Diagram for nearby stars atlasoftheuniverse/hr.html

HR Diagram for nearby stars http://www.atlasoftheuniverse.com/hr.html. Temperature. Main Sequence H burning pp/CNO exhaust core H Contraction Density/T inc. H shell burning Expansion Core He burning He shell burning. What happens at hydrogen exhaustion.

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417 views • 32 slides
HR Diagram for nearby stars atlasoftheuniverse/hr.html

HR Diagram for nearby stars atlasoftheuniverse/hr.html

HR Diagram for nearby stars http://www.atlasoftheuniverse.com/hr.html. Temperature. Main Sequence H burning pp/CNO exhaust core H Contraction Density/T inc. H shell burning Expansion Core He burning He shell burning. What happens at hydrogen exhaustion.

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473 views • 32 slides
Neutrinos and Supernova Nucleosynthesis: Importance for Astronomy and Cosmochemistry

Neutrinos and Supernova Nucleosynthesis: Importance for Astronomy and Cosmochemistry

Neutrinos and Supernova Nucleosynthesis: Importance for Astronomy and Cosmochemistry. Bradley S. Meyer Clemson University. Standard Picture. 92,94 Mo: p process 95 Mo: r, s processes 96 Mo: s process 97,98 Mo: s, r processes 100 Mo: r process. Motivation to Restudy 92,94 Mo synthesis.

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Study of the s-process in low mass stars of Galactic disc metallicity

Study of the s-process in low mass stars of Galactic disc metallicity

Study of the s-process in low mass stars of Galactic disc metallicity. Laura Husti Roberto Gallino Sara Bisterzo. Outline: Origin of the heavy elements. Stellar Nucleosynthesis and Evolution. S-process nucleosynthesis in AGB stars at solar metallicity.

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The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on

The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on

The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on a. observations of globular clusters. b. observations of open clusters. c. 21-cm radiation from H I regions. d. the rotation curve of the galaxy. e. the energy produced by Sagittarius A*.

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366 views • 5 slides

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