Evaluationof TVDhighresolutionschemes for unsteady viscous shocked¯ows VirginieDaru a ,ChristianTenaud b, * a ENSAM,Lab.Sinumef,151Bddel'Hopital,75013Paris,France b…
Slide 1Transition Oxford/Slow Food Chris Goodall 20 th November 2008 Why do global land use patterns matter so much? Slide 2 The purpose of this talk: To show that the conflict…
Slide 1Seismology and Earth’s Interior Slide 2 Mass of the Earth Spherical masses behave as if all mass located at central point g = GMe/R 2 Me = gR 2 /G g = 9.8 m/sec…
Slide 1 Temperature Luminosity What is a Hertzsprung- Russell diagram? An H-R diagram plots the luminosity and temperature of stars Slide 2 Most stars fall somewhere on the…
Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…
Type I Supernovae Eric LeJeune Supernova High-mass star’s final brilliance Star explodes A turning off or sudden turn on of nuclear fusion Classifying Type I & Type…
A105 Stars and Galaxies ROOFTOP TONIGHT AT 9 PM HAND IN HOMEWORK Exam coming on Nov. 2 Today’s APOD Upcoming Events Orionid meteor shower peaks Saturday night, view from…
Stellar Evolution The Mass-Luminosity Relation Our goals for learning: How does a starâs mass affect nuclear fusion? How does a starâs mass affect nuclear fusion? Stellar…
Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…