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Distant Galaxies

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Title: Distant Galaxies


1
Distant Galaxies
Edwin Hubble Measured distances to
galaxies Combined that with galaxy velocities
Came up with the Hubble Diagram
2
Vel. km/s
Velocity is proportional to distance v Ho d
Hubbles Law Ho slope Hubble Constant
Distance (Mpc - Megaparsecs)
3
  • Importance of Hubbles Law
  • Used to determine distances (d) (need velocity
    of a galaxy and the value of Ho)
  • What is Ho?
  • 70 km/s/Mpc.
  • 2. Why does the law exist?
  • The law exists because the Universe is Expanding!
  • 3. What does Ho measure?
  • Time
  • Hubbles Law can be used to study distant,
    younger galaxies and tells us how the Universe
    has/is evolving

4
Active Galaxies
Galaxies that are far away are younger
galaxies. Younger galaxies ? unsettled
galaxies Active Galaxies Large Energy
outputs Energy/Light given off at extreme
wavelengths Variable energy output Active
Galactic Nuclei Active galaxies - often younger
galaxies
5
  • BL Lacs Blazars
  • Characteristics
  • No spectra features
  • Non-thermal light
  • Seyferts Type I and II
  • Characteristics
  • Bright, variable core
  • Unusual spectra
  • Unusual energy output x-ray, IR, UV
  • High energy output

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Seyfert
Normal Galaxy
8
Radio Galaxies
Many galaxies produce radio light Galaxies that
produce A LOT of radio light Radio Galaxy Types
of radio galaxy sources - From the core From
external lobes (large structures)
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Quasars
Quasi-stellar objects (QSO) - Quasars Look like
stars (points) Unusual spectra - emission lines
of ??? 1963 Maarten Schmidt What if the
unidentified features were actual common
features? Spectra is unusual because of a high
redshift - high velocity away
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Quasars - high redshift spectra ? high
velocities Hubbles law high velocity ? great
distance Quasar are amongst the most distant
objects observed! Characteristics High
Velocity Great distance implied (by Hubbles
law) Not very faint ? very luminous Small
energy source Emission lines in spectra, often
broad
20
Model for Active Galaxies
BL Lac, Seyferts (I and II), Radio Galaxies,
Quasars All different? Or all the same? Could a
single model explain all of the features observed
in these active galaxies? What would be in this
model?
21
Black hole in center Accretion disk around
it High velocity clouds Low velocity clouds Dusty
torus (donut) Jets
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Gravitational Lensing
Einsteins General Relativity on a cosmic scale
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