XIII. Galaxies and the Structure of the Universe

1. Proof of other galaxies

Shapley - Curtis debate: nebulae in Milky Way or separate galaxies?

Hubble: Cepheids in galaxies (1924)

Period - Luminosity relation --> distance --> "island universes"

2. Galaxy types

a) Spirals

b) Ellipticals

c) Irregulars

d) Dwarf and faint galaxies

e) Why ellipticals and spirals? Still a riddle

  1. Not age - old stars in both
  2. Not rotation - won't cause lack of gas & dust in ellipticals
  3. Galaxies collide --> ellipticals

3. Masses of galaxies

a) Spirals

b) Ellipticals

c) Binary galaxies

d) Galactic clusters

Much more matter than observed in stars is needed to keep the structures together ! --> Dark matter problem everywhere

4. Galaxy Clusters

a) Local group

which our Milky Way galaxy and the Andromeda galaxy are in

b) Types of Clusters

Evidence in favor of scenario with collisions:

5. The Galactic Distance Scale and Huge Structures

a) Distances from combination of methods

b) Hubble's Law (1929)

Observed: Large redshift --> object far away

vaway = H x Distance (H: Hubble constant)

Hubble's Law can be used the other way around:

Redshift --> distance (galaxy map of universe)

c) Superclusters:the "Great Wall", sheets and voids (bubbles)

6. Active Galaxies

a) Radio galaxies

b) Seyfert galaxies

c) BL Lac objects

d) Quasars "quasi-stellar radio sources"

  1. Look star-like, but give radio (synchrotron), IR, UV, X, gamma
  2. Huge redshifts (Hubble)--> large distance
  3. Distance: If we see them --> huge luminosity
  4. Far away --> light needs long time --> objects in early universe
  5. Time changes --> energy generated in small regions
  6. Quasars = cores of forming galaxies?

Importance: clues to how & when galaxies form
Energy generation: a riddle
Supermassive black holes?
Is black hole formation part of galaxy formation?

Chapter 14