'Galaxies' presentation slideshows

Universe Eighth Edition

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Antarctica December 2006

625 views • 54 slides

AGENDA

AGENDA. Discussion Adjourn *Dinner on Own. ABST RACTS. Rachael Beaton Checks & Balances: Testing the Distance Ladder Determination of the Hubble Constant

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Dark Matter/Dark Energy Do we need it? How Much? Where? What is It? Hans-Walter Rix January 28, 2004 Observing the Big B

685 views • 39 slides

Exam

Exam. Final Exam: * Tuesday Dec 9 th @ 9am E2-229 EIT Complex * 2 hours. Only Specified Calculators! Recall notice from Faculty of Science: could end up with F-DISC in the course. (Can do questions without calculator.). ~70 questions in 2 hours About 10 math questions

683 views • 36 slides

Astro-2: History of the Universe

Astro-2: History of the Universe. Lecture 2; April 6 2006. Previously.. On Astro-2. The goal of cosmology is to understand how the universe formed and evolved. How can we build a theory of the universe valid at all times in every place?

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427 views • 33 slides

Spiral Galaxies

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Objectives: 1) To learn about Spirals 2) To learn about Barred Spirals

Goal: To know the different types of galaxies and to understand their differences and similarities. Objectives: 1) To learn about Spirals 2) To learn about Barred Spirals 3) To learn about Elliptical Galaxies 4) To learn about Irregular Galaxies. What type of galaxy is this?.

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GIANT TO DWARF RATIO OF RED-SEQUENCE GALAXY CLUSTERS Abhishesh N Adhikari Mentor-Jim Annis Fermilab IPM / SDSS August 8,

GIANT TO DWARF RATIO OF RED-SEQUENCE GALAXY CLUSTERS Abhishesh N Adhikari Mentor-Jim Annis Fermilab IPM / SDSS August 8, 2007. OUTLINE OF TALK. Introduction to SDSS The physics of my project: Giant to Dwarf Ratio in Red Galaxy Clusters MaxBCG: A cluster detection algorithm

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Light Years, Important People, Galaxies

Light Years, Important People, Galaxies. 8 th Grade. WHAT IS A GALAXY?. A galaxy is a huge group of single stars , star systems, star clusters, dust , and gas held together by gravity. How big are galaxies?. The largest galaxies have more than a TRILLION stars.

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Announcements

Announcements. Grades for third exam are now available on WebCT Observing next week counts on the third exam. Quasars and Active Galactic Nuclei. Quasi-stellar objects Redshifts Variability Supermassive black holes Active Galaxies Reading 24.1-24.2, 23.2. Quasars.

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The X-ray Morphology and Spectra of Galactic Disks

The X-ray Morphology and Spectra of Galactic Disks Richard Owen, Bob Warwick University of Leicester X-rays from Nearby Galaxies Introduction We use XMM-Newton to analyze disk emission from a sample of nearby face-on spiral galaxies.

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Chapter 6 - Specific Case Study: Searching for Bent-double Galaxies

Chapter 6 - Specific Case Study: Searching for Bent-double Galaxies . Chandrika Kamath Center for Applied Scientific Computing Lawrence Livermore National Laboratory http://www.llnl.gov/casc/people/kamath. UCRL-PRES-145087: The work of Chandrika Kamath in Chapters 5, 6, and 7

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AGN FEEDBACK AND QUENCHING OF STAR FORMATION: A MULTIWAVELENGTH APPROACH

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On the Shoulders of Giants

On the Shoulders of Giants. Organization of the universe. THE UNIVERSE: 3 theories 1. Open, expands forever 2. Closed, like a saddle 3. expanding and contracting. Galaxies: contain stars, huge clouds of gas and dust (nebulae) which revolve around a nucleus. Three types.

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Galaxy Resarch Project

By Yulissa Mendez

312 views • 13 slides

Dark Energy & Dark Matter

462 views • 13 slides

Jay Taub Online Astronomy Class JT-101 Astronomy Basics

Jay taub provides online study material about our galaxy,solar system,black holes etc.for more info visit us @ jaytaub.net

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Monday October 1, 2012

173 views • 7 slides