Overheads for Lectures:

1
Overheads for Lectures Large Scale Kinematics
for Elliptical Galaxies Line-of-sight velocity
distributions Kinematically Distinct
Cores Properties of Disk/Spiral Galaxies I The
Milky Way Structure MW Bulge evidence for
bar-like nature MW Bulge Age and
Metallicity MW Bulge Kinematics
2
(No Transcript)
3
(No Transcript)
4
(No Transcript)
5
(No Transcript)
6
Kinematically Distinct Cores (KDCs)
(Bender et al 1988)
7
(Efstathiou, Ellis Carter 1992)
8
(No Transcript)
9
Freudenreichs galaxy model
10
The ratio I(l,b)/I(-l,b) - surface photometry
shows asymmetries in l that would occur if the
Galaxy were barred, with the nearer end of the
bar at positive l. Compare with model.
11
(No Transcript)
12
(No Transcript)
13
(No Transcript)