8/27/03LSU - AEI Astrophysics1 The Nonlinear Development of Instabilities in Rotating Stars and Binary Star Systems Joel E. Tohline & Juhan Frank Kevin.
X-Ray UltravioletVisibleInfraredRadio The Electromagnetic Spectrum and the Universe.
Summary of Astronomy Test 1 Review Kepler’s Laws Test 1 Review Spectra –Continuous –Absorption –Continuous Test 1 Review Compute distance to a star using.
Francis T. O’Donovan based on Infrared Spectroscopy of the Black Hole Candidate GRO J1655-40.
Analytical Classical Dynamics An intermediate level course.pdf
Life Cycle Of A Star By Miharu Furuta. Introduction In the night we see things we know as stars, but they’re not simple, they’re life is very complex.
The Jovian Planets Chapter 7. Topics Jupter, Saturn, Uranus, Neptune How do we know? Why do we care? What is common about the outer planets? What is peculiar.
The Origin of the Solar System. The Great Chain of Origins: Early Hypotheses 1) Catastrophic hypotheses Example: passing star hypothesis: Star passing.
The Origin of the Solar System Lecture 13. Homework 7 due now Homework 8 – Due Monday, March 26 Unit 32: RQ1, TY1, 3 Unit 33: RQ4, TY1, 2, 3 Unit 35:
Cuesta College Eclipsing Binary Project Briefing In support of an ongoing Eclipsing Binary Star Project Conducted by Thomas C. Smith (Dark Ridge Observatory)
What are GW’s ?? Fluctuation in the curvature of space time, propagating outward form the source at the speed of light Predicted by Einstein’s GTR Gravitational.
Binary Star Evolution Cevin Kroxall Stellar Atmosphere’s à la Pilachowski.
