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Lecture 5: Galaxies

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Galaxy Mergers and Cannibalism. Galaxy Mergers. Stars pass right by one another (do not collide! ... Galactic Cannibalism. Forms the dominant cluster member ... – PowerPoint PPT presentation

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Title: Lecture 5: Galaxies


1
Lecture 5Galaxies
  • Dr Michael Burton

2
The Structure of our Galaxy
  • How did we find out?
  • Herschels 18th Century map
  • Analogy lighthouses above the fog
  • Globular Clusters
  • RR Lyrae stars (pulsating red giants)
  • Flattened disk in shape of Spiral
  • 100,000 light years across, 300,000 million stars
  • Dust lanes in disk (young stars)
  • Central Bulge (old stars)
  • Halo (globular clusters)

3
Galactic Rotation
  • Rotation curve is constant with distance
  • V 250 km/s
  • There must be Dark Matter (unseen matter
    exerting a gravitational pull)
  • Winding of spiral arms dilemma
  • Density Wave (cf. traffic jam on highway)
  • Star formation induced by compression of gas
    clouds as they pass through the spiral arm

4
The Realm of Galaxies
  • Island universes or nebulae in our Galaxy?
  • The Great Debate on the Scale of the Universe
  • Spirals galaxies
  • active star formation (young and old stars).
  • Elliptical galaxies
  • no gas, star formation has finished (all old
    stars).
  • Irregular galaxies
  • ill-defined shape

5
The Expansion of the Universe
  • Measure distance of galaxy
  • e.g. apparent size, brightness of supernova
  • Measure velocity of galaxy
  • Doppler shift
  • Hubbles Law
  • Speed H0 x Distance
  • H0 is Hubbles Constant
  • 71 ? 4 kilometres per second per megaparsec
  • (megaparsec million parsecs 3 million light
    years)
  • 1 / H0 age of Universe (13.7?0.2 billion years)

6
Galaxy Clusters
  • Milky Way is in the Local Group
  • a small cluster of galaxies
  • Galaxies are clustered.
  • Clusters combine to form superclusters.
  • Large Scale Structure (e.g. the Great Wall)
  • 2dF instrument on the AAT has measured 250,000
    galaxies.

7
Galaxy Mergers and Cannibalism
  • Galaxy Mergers
  • Stars pass right by one another (do not collide!)
  • Gas collides, induces star formation
  • Galactic Cannibalism
  • Forms the dominant cluster member
  • Galaxies today built up by mergers over first 12
    billion years of the Universe.

8
Galaxy Formation
  • Hubble Deep Field
  • a pencil beam to the early universe
  • We see the building blocks of galaxies, merging
    together and undergoing star formation
  • Theories for Galaxy Formation
  • Collapse of a single huge gas cloud?
  • Coalescence of many smaller clouds?
  • Perhaps a bit of both??

9
Quasars andActive Galactic Nuclei
  • Central engine a supermassive black hole
  • Surrounded by accretion disk
  • Emitting jets of plasma at relativistic speeds

10
The Story of the Universe
  • MAP satellite measures the Cosmic Microwave
    Background Radiation
  • Pins down tightly several parameters that
    describe the nature of our Universe
  • The Universe is 13.7?0.2 billion years old
  • The Universe will expand for ever
  • Ordinary matter only makes up 4 of it
  • Dark Matter is 23, Dark Energy is 73
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