In Search Of_Dark-matter ~ tsg
In search of dark matter
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (University of Pretoria)
Lecture 2: Spaceship Earth Man is…related inextricably to all reality, known and unknowable…plankton, a shimmering phosphorescence on the sea and the.
Slide 1 The Family of Stars Chapter 9. Slide 2 Part 1: measuring and classifying the stars What we can measure directly: – Surface temperature and color.
Lecture 2. Examination The course is assessed in three parts: Problem sets. The problem sets and the peer reviews. One of the sets will randomly be corrected.
Lee Hartmann, University of Michigan
11 th Lec Phase Space. Collisionless Systems We showed collisions or deflections are rare Collisionless: stellar motions under influence of mean gravitational.
KIAA Lectures Beijing, July 2010 Ken Freeman, RSAA, ANU Lecture 4: stellar data - sources and techniques.
17-1 How we can measure the distances to the stars 17-2 How we measure a star’s brightness and luminosity 17-3 The magnitude scale for brightness and.
Black Hole Mimickers Daniela Pérez and Gustavo E. Romero Instituto Argentino de Radioastronomía (IAR-CCT CONICET) Texas in Geneva, December 17, 2015 Contact:
Galaxy Formation and Evolution Galactic Archaeology Chris Brook Modulo 15 Room 509 email: [email protected].
