Astronomy 406
Lecture 16, Oct. 2
Fall 2013
Lecture Notes:
pdf file
Our Supermassive Black Hole: Sgr A
*
The trouble with ground-based
observations
and the power of
adaptive optics
using
laser
guide stars
Stellar orbits:
Munich group
,
UCLA group
; orbits in
3D!
Implications
Milky Way quiescence versus activity of, e.g.,
M87
Ongoing: Galactic weather
forecast
:
infall
of
gas clouds
the future: resolving the shadow with the
Event Horizon Telescope
the
VLBI
technique
expectations: will we see
this?
hypervelocity stars
such as
this one
Globular Clusters
Vital statistics
Exemplars
M3
,
zoom
47 Tuc
,
zoom
omega Cen
and its
center
M15
cluster
discovery
in Galactic plane
Structure:
density profiles
Classes
Globular Cluster HR Diagrams
example
(
source
)
Colorized
schematic
H-R diagram
animation
--watch 'em evolve!
another
animation
Theory fits:
isochrones
= HR curves for different ages (
source
)
Tides and Stripping
Tidal forces
Tidal stripping
Caught in the act
globular cluster
Palomar 5
the
Magellanic stream
at
21 cm
interacting
galaxies
Virial Theorem
Globular Cluster Evaporation
Lecture Archive
Brian D. Fields
Last modified: Wed Oct 2 16:01:40 CDT 2013