'Red giant stars' presentation slideshows

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This page is intentionally blank. Forging the elements. Tales of the Sun and stars. A new view of the Universe IV Fred Watson, AAO, with thanks to Jessica Chapman, ATNF April 2005. Main Sequence Stars and Beyond. Our sun as a star Nuclear fusion and the main sequence

625 views • 50 slides

Reaction Rates

Reaction Rates. Marialuisa Aliotta. School of Physics University of Edinburgh. principles of stellar structure and evolution general features of thermonuclear reactions experimental approach. Second European Summer School on Experimental Nuclear Astrophysics

569 views • 48 slides

Detection of a Large-Scale Structure of Intracluster Globular Clusters in the Virgo Cluster

Detection of a Large-Scale Structure of Intracluster Globular Clusters in the Virgo Cluster ???? ???? ??? ????? ???? ?? (Lee, Park , & Hwang 2010, Science) ??? (Park, Hong Soo) ????????? 2010. 3. 24 ??????? ????. Contents 1. Introduction 1.1 Properties of GCs

560 views • 45 slides

The Life Cycle of Stars Power Point Maze V2.0

The Life Cycle of Stars Power Point Maze V2.0. How much do you know?. Rules of the Game. You will compete in team sizes of your teachers determination. Players are allowed to participate twice only after all other students have played.

486 views • 39 slides

Chapter 30 Section 2 Handout

Chapter 30 Section 2 Handout. Stellar Evolution. 1. Why are astronomers not able to observe the entire life of any star? Because a star typically exists for billions of years. 2. What is luminosity? The total amount of energy a star gives off each second. 3.

523 views • 37 slides

Chapter 30 Section 2 Handout

Chapter 30 Section 2 Handout. Stellar Evolution. 1. Why are astronomers not able to observe the entire life of any star? Because a star typically exists for billions of years. 2. What is luminosity? The total amount of energy a star gives off each second. 3.

483 views • 37 slides

290 views • 29 slides

15-3

15-3. The Lives of Stars. Studying the Lives of Stars. Astronomers must study stars at different stages to study the lives of stars. A star is born. Stars are born in nebula (a vast cloud of gas and dust) Gravity pulls gas together When nuclear fusion takes place a star is born

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A Deep Photometric Study of M83 with the DuPont and Magellan Las Campanas Telescopes

A Deep Photometric Study of M83 with the DuPont and Magellan Las Campanas Telescopes. Bryan Penprase (Pomona College), Barry Madore, Wendy Freedman (OCIW), and Ryan Quadri (Yale). Abstract:

98 views • 2 slides