Astronomy 406
Lecture 9, Sept. 16
Fall 2013
Lecture Notes:
pdf file
Research Opportunties: Prof.
Ryan Foley
Mapping the Milky Way: Gas and Dust
neutral atomic hydrogen (H I):
21-cm hyperfine emission
molecular hydrogen
(really:
CO molecules
)
ionized hydrogen (really: H-alpha recombinations;
northern
sky from
WHAM
,
southern
sky from
SHASSA
,
all-sky
)
all hydrogen
(really:
high-energy gamma-rays
)
warm dust (as seen in the
far infrared
)
Mapping the Milky Way: Stars
Global optical view:
Tycho-2 map
of brightest 2.5M(!) stars in B and V
Truly global view:
near infrared
Stellar disk (Population I): thin, thick
Spheroid (Population II): stellar halo, bulge
cartoon
of Milky Way structure
A Census of Local Stars
the
151 (apparently) brightest stars
RECONS
data on the
100 nearest stars
biases in star surveys
the present-day
luminosity function
Lecture Archive
Brian Fields
Last modified: Mon Sep 16 10:43:01 CDT 2013