Astronomy 406
Lecture 5, Sept. 6
Fall 2013
Lecture Notes:
pdf file
Update! Closest star system found in the past century
press release
Luhman (2013)
article
The Hertzsprung-Russell Diagram
real data: Hipparcos
unlabelled
,
labelled
observer's version
(i.e., axes in observational units)
theoretical version
(i.e., axes in underlying physical units)
Stars: More Physical Properties
Mass: from
binary systems
visual binaries:
Mizar orbit
spectroscopic
binaries
Mass-luminosity relation
plotted
for main sequence stars
implications for
HR diagram
HR diagram
comparison
: nearest vs brightest (highest flux) stars
implications for galaxies:
spiral
vs
elliptical
Stellar Stability
gasses and pressure
java applets:
kinetic theory
,
gas law
,
piston
,
ideal atmosphere
hydrostatic equilibrium
stability
solar response to
flare
Stars in a Nutshell
stellar structure
star birth:
Eagle nebula
starburst
galaxy
stellar
spectra
: a
digitial classification atlas
the main sequence: nuclear reaction chains
Super-K
and its
image
of the Sun, in
neutrinos
H-R diagram
animation
--watch 'em evolve!
another
animation
post-main sequence evolution
low mass:
M dwarfs, L dwarfs and T dwarfs
; an
L dwarf
discovery in IR
intermediate mass:
red giants
planetary nebulae:
Cat's eye nebula
,
spirograph nebula
white dwarfs:
cool!
implications: near-IR Milky Way
K giants
elliptical galaxy NGC 2768
high mass:
supergiants:
Betelgeuse
supernovae:
1987A
,
1999em
,
2005cs
ejecta:
N63A
neutron stars and pulsars:
Crab nebula
black holes:
Cyg X-1
nucleosynthesis:
the
periodic table
and
the circle, the
circle of life
Lecture Archive
Brian Fields
Last modified: Wed Sep 4 10:39:58 CDT 2013