Caption:
An animation of
"stochastic self-propagating star formation (SSPSF)
simulated in a simple circular model" of a
flocculent spiral galaxy
seen
face-on.
The mechanism that creates
flocculent spiral arms
is believed to be
stochastic self-propagating star formation (SSPSF).
Self-propagating
star formation is discussed in
IAL 21:
Star Formation: The Evolution of Star Formation Regions.
In brief, this is the story of
stochastic self-propagating star formation (SSPSF)
and
flocculent spiral arms:
- There is a large molecular cloud
in which star formation is triggered in one part.
- Massive
OB stars (AKA hot young blue stars) form.
Their radiation pressure
and stellar winds
and the ejecta from their
supernova explosions
compress nearby regions of the molecular cloud.
- This compression triggers a new generation of
star formation
adjacent to the original one, where
star formation
is tending to turn off because the
ultraviolet light
(fiducial range 0.01--0.4 μm)
from the OB stars is
evaporating the interstellar dust
and cloud
material is being pushed away the same pressure forces that
trigger the adjacent star formation.
- Thus star formation
self-propagates through the large
molecular cloud.
- But the molecular cloud
is so large that it is differentially
revolving around the
galaxy
center of mass.
In most galaxies, the orbital speed (measured in, e.g.,
km/s) is fairly constant
(due their dark matter halo
mass distribution), but this means that the
angular velocity
(measured in, e.g., in degrees
per megayear (Myr))
falls off with radius from the
galaxy
center of mass.
- Thus, as one goes outward in radius, the
molecular cloud material
is increasingly trailing.
- The molecular cloud
is getting wound up and is forming
spiral arms.
- But the
winding-up problem
(see Galaxies file:
spiral_arm_winding_problem.html)
NEVER arises, because the
molecular cloud
disperses in a complex way after a few tens of
megayears and the orbital periods
of the material is of order hundreds of megayears.
- Because
star formation regions
are NOT formed by organizing
spiral density waves,
the
star formation regions
formed by
stochastic self-propagating star formation (SSPSF)
ARE messy, and so the
spiral arms formed are messy:
they are the
flocculent spiral arms.
Credit/Permission: ©
User:JanRosseau,
2018 /
CC BY-SA 4.0.
Image link: Wikimedia Commons:
File:SSPSF simulation.gif.
Local file: local link: stochastic_self_propagating_star_formation.html.
File: Galaxies file:
stochastic_self_propagating_star_formation.html.