KITP: collapse

This beautiful tuesday morning, Dave tutors us on relaxation and cluster core collapse.
Then it is party at Alison's place.

But, first, we go through thermodynamics of self-gravitating internally relaxed systems, multiple equilibria and general dimensionless solutions.



Open Cluster M7 (from Utahskies.org)



Globular cluster M4 (from Utahskies.org)

Core collapsed? Or not?



Globular cluster M15 (from Utahskies.org - ok actually hubblesite, but they had a scaled copy and I was on a roll)

Definitely core collapse, we think.

Seriously - there are more core collapsed or post-core collapsed clusters in the inner parts of the galaxy, as there should be, we think, maybe, depending on your definition.

M15 really almost certainly is in post-core collapse bounce, it is the only sensible way to explain PSR M15C and many other things about it.

But M4?
Which is it? A nice pre-collapse King model cluster?
Or a strongly modified way past post-core collapse cluster...?



ω Cen - absolutely positively definitely NOT a globular cluster

ω Cen is a nuisance, it violates all precepts about globulars, except how it looks,
ergo, it is not a globular
right?

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Today we step back and Hans runs The Big Questions past us. It is always good to think about the Big Picture. The Big Questions
LTP activated genes are clustered on chromosomes -- or so says some work by Park et al in JBC.
it is still raining?! so we have an east coaster telling us about actual data on x-ray binaries in clusters, globular clusters in other galaxies...
It seems like it was just last week that I wrote about colliding dark matter, showing what happens when two galaxy clusters collide.

"except how it looks, ergo, it is not a globular right?"

If it looks like a spherical cow, and moos like a spherical cow, it probably is a spherical cow.