Astronomy 210
Lecture 36, April 20
Spring 2018
Lecture Notes:
pdf file
Black Holes: Theory
Size and recipe
Black holes from afar, near, and
inside
Black hole
inspiral
and
collisions
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
coming soon(?):
Event Horizon Telescope
image of a black hole, perhaps like
this
,
this
, or
this
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
important clues: a binary supermassive black hole pairs and even
triples
! optical
detection
by our own
Prof. Xin Liu
,
X-ray
Gravitational Radiation
Theory: ripples in spacetime
Indirect evidence:
Hulse & Taylor's
award-winning
binary pulsar
Direct detection: gravity-wave observatories
Advanced
LIGO
: detectors in
Hanford
and
Livingston
VIRGO
: detector near
Pisa, Italy
the future:
LIGO India
,
KAGRA, Japan
,
LISA
Welcome to the era of
gravity
wave
astronomy!
merging
black holes
merging
neutron stars
Nobel Prize 2017
: Rainer Weiss, Barry Barish, Kip Thorne
Lecture Archive
Brian D. Fields
Last modified: Fri Apr 8 12:05:13 CDT 2011