Astronomy 404
Lecture 27, Oct. 27
Fall 2021
Lecture Notes:
pdf file
Convection in Stars
convective instability:
simulation
example:
granulation
in the Sun
condition for convection: temperature gradient
simulation
of a convective star
convection in main sequence stars
The Main Sequence Across Stellar Masses
trends summarized
importance of helium core and thus stellar mixing
Evolution Beyond the Main Sequence: Low Mass Stars
core degeneracy
shell hydrogen burning
red giant phase
Gaia HR diagrams:
field stars
,
globular cluster
Final Phases of a Solar Mass Star
helium flash
core helium burning
asymptotic giant branch
paths on
temperature-density diagram
(
Kovetz+ 2009
)
Planetary Nebulae
winds and mass loss:
Mira
resolved
, trailing
wake
planetary nebula ejection and illumination
observed planetary nebulae:
Ring Nebula:
optical
, zoom
out
lemon slice
NGC2022
helix
spirograph
Lecture Archive
Brian D. Fields