Astronomy 210
Lecture 37, April 25
Spring 2011
Lecture Notes:
pdf file
Evidence for Black Holes
X-ray
binaries
:
Cygnus X-1
Milky Way center:
Radio
overview
The power of
adaptive optics
Stellar orbits:
Munich group
,
UCLA group
possibly related: gamma-ray
bubbles
other galaxies
active galaxies:
M87
; AGN
gallery
gravitationally lensed quasar: the
Einstein cross
quasar and
host galaxies
supermassive black holes
black holes and galaxies somehow
know about each other
an important clue?
a binary supermassive black hole pair!
Gravitational radiation
Hulse & Taylor's
award-winning
binary pulsar
gravity-wave observatories:
LIGO
(operational) and
LISA
(future)
Changing Gears:
The Big Picture
Our Milky Way Galaxy
Our Place in the Milky Way
The naked eye
Milky Way
:
southern hemisphere
, zoom to
dark lanes
, more
bands
Galileo:
telescope
Immanuel Kant
William Hershel's
model
(top view)
Harlow Shapley
globular cluster
distribution: on the
sky
, in
space
interstellar dust:
microscopic view
, in a
dark cloud
and
reflection nebula
another
example
of scattering and absorption
simulated view
of Milky Way seen from outside; a possible similar
galaxy
Lecture Archive
Brian D. Fields
Last modified: Mon Apr 25 10:09:58 CDT 2011