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Classifying galaxies is hard, and different people do it different ways Except for nearby, we can only see bright galaxies I will ignore dwarf spheroidal.
Classifying galaxies is hard, and different people do it different ways Except for nearby, we can only see bright galaxies I will ignore dwarf spheroidal.
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Hidden lives v2
Hidden lives v2
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This animation begins with a collapsing interstellar cloud of gas and dust. Most of the material becomes part of the young Sun, but some debris.
This animation begins with a collapsing interstellar cloud of gas and dust. Most of the material becomes part of the young Sun, but some debris.
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Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked about how galaxies provide an environment for the stars.
Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked about how galaxies provide an environment for the stars.
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ACTIVE GALAXIES and GALAXY EVOLUTION Quasars, Radio Galaxies, Seyfert Galaxies and BL Lacertae Objects Immense powers emerging from ACTIVE GALACTIC NUCLEI:
ACTIVE GALAXIES and GALAXY EVOLUTION Quasars, Radio Galaxies, Seyfert Galaxies and BL Lacertae Objects Immense powers emerging from ACTIVE GALACTIC NUCLEI:
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USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1
USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1
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Introduction Active Galactic Nuclei Lecture -2- Taxonomy & Unification.
Introduction Active Galactic Nuclei Lecture -2- Taxonomy & Unification.
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ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections 0101-0106.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections 0101-0106.
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Dusty star formation at high redshift Chris Willott, HIA/NRC 1. Introductory cosmology 2. Obscured galaxy formation: the view with current facilities,
Dusty star formation at high redshift Chris Willott, HIA/NRC 1. Introductory cosmology 2. Obscured galaxy formation: the view with current facilities,
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Active Galactic Nuclei Thomas Schlenker University of Washington Department of Physics PHYS 496 -What is an AGN? -What kinds of AGN’s are out there? -Unified.
Active Galactic Nuclei Thomas Schlenker University of Washington Department of Physics PHYS 496 -What is an AGN? -What kinds of AGN’s are out there? -Unified.
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Jelle de Plaa Irina Zhuravleva, Norbert Werner Eugene Churazov, Jelle Kaastra, Yan Grange Turbulence measurements in two giant elliptical galaxies.
Jelle de Plaa Irina Zhuravleva, Norbert Werner Eugene Churazov, Jelle Kaastra, Yan Grange Turbulence measurements in two giant elliptical galaxies.
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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.
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.
215 views