PPT-Chap 17-18: Stellar Evolution – the Life and Death of a Star…

Chap 1718 Stellar Evolution the Life and Death of a Star Heres the story well tell Lowest mass stars and their evolution Low mass star evolution High mass star evolution Stellar death and stellar corpses. Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . . Natalia Storch, Kassandra Anderson & Dong Lai. Cornell University. Many hot Jupiter systems . have . been found to exhibit misalignment between the . orbital axis (. L. , the axis perpendicular to the orbital plane) . 1. /28. Important for transits (see next slides).. . Transit depth = [ . R. planet. (. λ. ,t. ) / . R. star. (. λ,t. ) ]. 2. Not so important for eclipses because the eclipse is a simple difference, and the stellar variability typically is slower than the eclipse: . 1. Interblocage = impasse (Deadlock). Chapitre 8. http://w3.uqo.ca/luigi/. Chap 8. 2. Interblocages: concepts importants. Caractérisation: les 4 conditions. Graphes allocation ressources. Séquences de terminaison. 1. Module 10 – Structure de mémoire de masse (disque). Chapitre . 10 (. Silberschatz. ). Chap. 10. 2. Concepts importants du Module 10. Fonctionnement et structure des unités disque. Calcul du temps d’exécution d’une séquence d’opérations. Interpolating Values. Animation(U), Chap 3, Interpolating Values. 1. 2. Outline. Interpolating/approximating curves. Controlling the motion of a point along a curve. Interpolation of orientation. Working with paths. Key variable is . mass. of star. directly measured only for binary stars, but it determines position on main sequence. Cluster ages. Main-sequence luminosity increases . much. faster than mass. therefore massive stars use up their fuel much faster. Wen-Ping . Chen . National . Central . University . Census of Galactic open clusters. . Dynamical evolution of a star cluster. . Star clusters as targets and as tools. Outstanding issues. 2017 April 28 PMO . Revision . lecture. Lecture slides available in . powerpoint. and . pdf. from. www.star.le.ac.uk. /~. mbu. /. lectures.html. Everything taught in the course is examinable…... However, here is a crib sheet of what to focus on. Chap 5-. 1. Chapter 5. Discrete Probability Distributions. Basic Business Statistics. 12. th. Edition. Chap 5-. 2. Copyright ©2012 Pearson Education, Inc. publishing as Prentice Hall. Chap 5-. 2. Learning Objectives. Chap 16-. 1. Chapter 16. Time-Series Forecasting. Basic Business Statistics. 12. th. Edition. Chap 16-. 2. Copyright ©2012 Pearson Education, Inc. publishing as Prentice Hall. Chap 16-. 2. Learning Objectives. FALL . 2018. 2018. Chap. 12 -- Privileges. 2. DEFINITION. A PRIVILEGE IS A RIGHT OF SOME PERSON OR ENTITY TO BLOCK THE ADMISSION OF CERTAIN KINDS OF EVIDENCE IN A CASE. EVEN THOUGH RELEVANT. EVEN THOUGH CRUCIAL. Prof. JANICKE. 2018. Evid. Intro. Chap. 1. THE SUBJECT IS:. A BODY OF RULES, TELLING LAWYERS WHAT THEY CAN AND CAN’T (MOSTLY) DO TO . ESTABLISH FACTS. AT TRIAL. “LAW” POINTS ARE ESTABLISHED DIFFERENTLY; NO RULES OF EVIDENCE APPLY. Laura . Magrini. INAF- . Osservatorio. . Astrofisico. di . Arcetri. In Our Galaxy. Open clusters (disc population): . Many (~2200 known clusters). . even more new candidates in the inner disc from infrared surveys .