XII. The Milky Way
1. Structure of the milky way
a) See band of stars in the sky we are in disc full of stars
b) Distance determination
- use distance of stars to get spatial
distribution
- (spectroscopic parallax (HR diagram))
Kapteyn concluded: We are in the center!
c) Galactic Halo
- Shapley used Globular clusters
- Distance from Cepheids in globulars 3D
map (1917)
Galactic Halo consists of:
- Globular clusters (old Population II
stars) Left over from pre-galactic-collapse
- Individual Population II stars, high
velocities (ejected from globulars?)
- 21 cm hydrogen gas
d) Spiral structure
- The Milky Way has features in common
with other spiral galaxies:
- Flat disc (rotation)
- Emission nebulas (red) and 21 cm -->
H gas
- Radio maps of Milky Way show spiral structure:
- spirals would wind up after a few rotations
- but: galaxy > 20 rotations -->
not the same material in arms
- Young hot (blue) stars light up arms:
- density waves --> compression
--> more self-gravity --> star
formation
- Dust
2. Mass of the galaxy
a) Mass from motion of star clusters
- Doppler shifts of globulars etc. -->
"galactic rotation curve"
- Velocity does not fall off with distance
from center
- i.e. non-Keplerian orbits --> most
mass outside disc(not seen in stars)
- missing
mass problem.
b) Galactic corona
- Observed:
- UV absorption lines --> hot (ions)
and turbulent (Doppler) gas
- Most mass of galaxy? -->
missing mass ?
- What kind?Brown Dwarfs? Black Holes?
Strange form of Matter?
3. Galactic center:
Exciting observations:
- Expanding & rotating rings (Doppler
effect) --> explosions in center?
- Synchrotron radiation "blob" near center
--> explosion?
- SgrA* - small intense radio source
- Need 3 x 106 Msun in SgrA* to keep things
from flying away
- SgrA* = supermassive black hole (~H100
Msun)?
- Rotating (Doppler) molecular disc around
SgrA*
- Matter falling in --> energy to power
all the bizarre features?
- Gammas from electron-positron annihilation
- Other galaxies: rapid central rotation
--> supermassive black holes?
Chapter 13