PPT-Chap 20,21: Galaxies – Classifications, Evolution
Author : aaron | Published Date : 2018-11-03
Heres the Story Well Unfold for You Hubbles galaxy classifications Spirals ellipticals irregulars Structural parts of galaxies disk halo nucleus bulge Spiral
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Chap 20,21: Galaxies – Classifications, Evolution: Transcript
Heres the Story Well Unfold for You Hubbles galaxy classifications Spirals ellipticals irregulars Structural parts of galaxies disk halo nucleus bulge Spiral arms tracers of star formation. Thorsten Naab . MPA, . Garching. . What regulates galaxy formation? . Leiden, April, 22. nd. How do massive galaxies get their gas and stars?. Gas accretion involves dissipation – energy can be radiated away . D.J. Pisano. (West Virginia University). Why study galaxy environment?. Nature vs. Nurture. Can they be distinguished?. What does the environment do to a galaxy?. What would a galaxy look like without any environmental influence?. With a wide-field multi-IFU spectrograph. Cluster studies. Clusters provide large samples of galaxies in a moderate field. Unique perspective on the interaction of galaxies with their environment. As they operate much as a closed box, they are useful as tracers of galaxy evolution and of cosmology. Exercise . 20.16. Add . the operation commit at the end of each of the transactions T 1 and T 2 from. Figure . 20.2. ; then list all possible schedules for the modified transactions.. Determine which of the schedules are recoverable, which are . 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. 1. Chapitre 10. Mémoire virtuelle. http://w3.uqo.ca/luigi. /. Virtuelle . est . une ressource d’ordinateur . qui n’est pas . offerte directement par le matériel. , elle est créée par le logiciel. 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. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Prof. JANICKE. 2018. 2018. Chap. 8 -- Impeachment. 2. DEFINITION AND METHODS. IMPEACHMENT IS THE PROCESS OF ATTEMPTING TO WEAKEN THE PERCEIVED CREDIBILITY OF A WITNESS. MOST COMMONLY DONE ON CROSS. AT LEAST SIX METHODS OF IMPEACHMENT, EACH WITH ITS OWN RULES LIMITING REACH. Prof. JANICKE. 2018. 2018. Chap. 13 -- Authentication. 2. AUTHENTICATION. A SUBSET OF RELEVANCE. AUTHENTICATION EVIDENCE IS. NEEDED BEFORE DOCUMENTS AND TANGIBLE THINGS ARE RECEIVED IN EVIDENCE. NOT NEEDED FOR TESTIMONY. 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. P. JANICKE. 2018. ONLY “STATEMENTS. ” . CAN . BE . HEARSAY EVIDENCE – . CAN’T BE REVEALED IN COURT. MUCH HUMAN DISCOURSE IS NON-STATEMENT. 3. statements. UTTERANCES. MEANINGS. UTTERANCE = ANYTHING WE SAY OR WRITE. 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 .
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