'Early types' presentation slideshows

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Databases & SQL

Databases & SQL

Databases & SQL. Teacher: Henny Klein email E.H.Klein@rug.nl contact: wednesday 14-16 room 11 - 426. All material and assignments on Nestor. First block C H 1 t.m. 5 Basic knowledge for the design and manipulation of relational databases Second block C H 6 t.m. 10

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372 views • 30 slides
The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA

The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA

The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA. Collaborators:. GEMS team (Chien, Hans-Walter, Klaus, Rachel + 15). Lutz Wisotzki, Malte Schramm, Bernd Husemann (AIP) Geraldine Letawe, Pierre Magain (Liege), Frederic Courbin (Lausanne) + 5.

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430 views • 26 slides
The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA

The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA

The properties of AGN host galaxies: Any clues for AGN feedback? Knud Jahnke, MPIA. Collaborators:. GEMS team (Chien, Hans-Walter, Klaus, Rachel + 15). Lutz Wisotzki, Malte Schramm, Bernd Husemann (AIP) Geraldine Letawe, Pierre Magain (Liege), Frederic Courbin (Lausanne) + 5.

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281 views • 26 slides
Galaxies and their Environments

Galaxies and their Environments

Galaxies and their Environments. Nick Cowan UW Astronomy January 26, 2007. Reasonable Questions. Why care about environments? What is an environment? How do we determine environments? How exactly do environments effect galaxies?. Galaxy Environments.

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368 views • 20 slides
Short GRBs: spectra & redshifts

Short GRBs: spectra & redshifts

Short GRBs: spectra & redshifts. G. Ghirlanda Osservatorio Astronomico Brera giancarlo.ghirlanda@brera.inaf.it. in collaboration with:.

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287 views • 19 slides
Old Stellar Populations in Galaxy Clusters

Old Stellar Populations in Galaxy Clusters

Old Stellar Populations in Galaxy Clusters. Scott Trager (Kapteyn Institute, Groningen) with Sandy Faber (UCO/Lick) Alan Dressler (Carnegie Observatories). Introduction: Why Cluster Galaxies?. Why early-type galaxies?

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366 views • 19 slides
HEROs in an Overdense Region at z=2.4

HEROs in an Overdense Region at z=2.4

HEROs in an Overdense Region at z=2.4. Myungshin Im (Seoul National University) & IRAC GTO team (PI: G. Fazio) Partial List of Collaborators: M. Pahre, H. Smith, S. Willner (SAO) + IRAC GTO. M. Lacy, F. Marleau, D. Fadda (SSC). What is HERO?.

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300 views • 19 slides
MONEY MONEY MONEY

MONEY MONEY MONEY

MONEY MONEY MONEY. DEATH TO PENNIES. http://www.youtube.com/watch?v=y5UT04p5f7U. History of Money: Timeline. http://www.pbs.org/wgbh/nova/ancient/history-money.html Discussion What are some early types of currency? What was the most surprising about the history of money?

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395 views • 9 slides
Technical Developments and Cultural Trends in Sport

Technical Developments and Cultural Trends in Sport

Technical Developments and Cultural Trends in Sport. Historical Perspective. Historically sport was for entertainment, participants could receive money for competing and betting was common. Commercialisation of sports began in the 19 th century following the industrial revolution.

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222 views • 9 slides

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