What is the center of a globular clusters made of?

Click For Summary

Discussion Overview

The discussion revolves around the composition and characteristics of the centers of globular clusters, exploring whether they contain stars, black holes, or other structures. Participants also delve into the formation of globular clusters and their gravitational binding to the Milky Way, touching on various theoretical and observational aspects.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants question whether the center of a globular cluster is a star or a black hole, with one suggesting that it could be mainly empty space.
  • There is mention of the possibility of black holes at the centers of globular clusters, with references to specific clusters like M15 and Mayall II that may host intermediate-mass black holes.
  • Participants discuss the high star density in globular clusters and how close interactions can lead to the formation of exotic stars like blue stragglers.
  • One participant raises the question of how globular clusters remain tightly bound over billions of years, contrasting them with open clusters that have much shorter lifetimes.
  • There are speculations about whether globular clusters could be remnants of larger, more distended objects that have been tidally stripped down.
  • Some participants express interest in the observational capabilities regarding the resolution of individual globular clusters at cosmological distances.
  • There are discussions about the gravitational dynamics within globular clusters and how mutual attraction among stars contributes to their stability.
  • One participant conjectures about the formation of globular clusters in relation to the formation of galaxies, suggesting a "bottom-up" coalescence process.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the composition of globular cluster centers, the presence of black holes, and the mechanisms that maintain their stability. The discussion remains unresolved with no consensus reached on these points.

Contextual Notes

Participants note the complexity of gravitational interactions within globular clusters and the challenges in observing their structures at cosmological distances. There are also references to specific observational studies and theoretical models that remain open to interpretation.

Who May Find This Useful

Individuals interested in astrophysics, particularly in the dynamics and formation of star clusters, as well as those exploring the relationship between globular clusters and galaxies.

  • #31
wabbit said:
Look at the sun through a solar filter.
solar filters come in all variations of colour renditions ... that's a very poor comparison
 
Astronomy news on Phys.org
  • #32
see where the sun is on the standard H-R diagram ...

H-R%20Diagram1.jpg
 
  • #33
davenn said:
solar filters come in all variations of colour renditions ... that's a very poor comparison
Yes but good ones have a flat transmission curve. See for instance http://www.alpineastro.com/Solar_Observation/Images/DERF_Curve_Lg.jpg
 
  • #34
davenn said:
see where the sun is on the standard H-R diagram ...

View attachment 79343
Yes G2 star. The colors on his chart are illustrative,not accurate.
 
  • #35
accurate enough to give a good indication compared to the other stars in the sequence and you will find that is the description in most places
 
  • #36
davenn said:
not sure where you get that from ?
That the range goes red white blue ? You can call it red yellow white bluish if you prefer : )
 
  • #37
wabbit said:
Yes but good ones have a flat transmission curve. See for instance http://www.alpineastro.com/Solar_Observation/Images/DERF_Curve_Lg.jpg

I haven't seen one yet that doesn't change the colour of what is being viewed
 
  • #38
believe what you like
I have had enough of your argumentative attitude !
I have put you on ignore
 
  • #39
davenn said:
I haven't seen one yet that doesn't change the colour of what is being viewed
Try Baader they ain't bad
 
  • #40
liometopum said:
Dr. William Harris, and his Ph.D. student, Jeremy Webb, of McMaster University, wrote an article for Astronomy magazine, July 2014, titled "Life Inside A Globular Cluster".
Very nice! especially the view from apogalacticon
 
  • #42
You can see the view from different locations within a globular cluster at Jeremy Webb's page,
http://www.physics.mcmaster.ca/~webbjj/liagc.html
Three images:
1. View from the center
2. View from near the half-light radius of the cluster
3. View from apogalacticon
 
Last edited by a moderator:
  • Like
Likes   Reactions: Bandersnatch
  • #43
Here is a link to a globular cluster lecture by Dr. William E. Harris of McMaster University.
http://physwww.mcmaster.ca/~harris/mcgill09aug.pdf

He covers a number of interesting things, among them being:
The Milky Way has 150 GCs
The Sombrero galaxy has about 1900 GCs
Discusses the size distribution of GCs
Formation via Young Massive Clusters in starburst dwarf galaxies
Some have black holes, and some do not
Globular clusters evaporate (the stars leave the GC). They all evaporate, except the big ones take a long time to do so.
 
  • Like
Likes   Reactions: TEFLing
  • #44
liometopum said:
You can see the view from different locations within a globular cluster at Jeremy Webb's page,
http://www.physics.mcmaster.ca/~webbjj/liagc.html
Three images:
1. View from the center
2. View from near the half-light radius of the cluster
3. View from apogalacticon
cool link and nice artistic impressions :smile: thankyou

I think it would be amazing to be able to look down on the Milky Way from above the galactic plane from such a "close" distance,
rather than from edge on as we currently do

The last image gives a hint of that view :smile:

Dave
 
Last edited by a moderator:
  • #45
liometopum said:
Globular clusters evaporate (the stars leave the GC). They all evaporate, except the big ones take a long time to do so.

Yeah, I would suggest a very long time. Spectral analysis of GC stars indicate that many of them are very old stars
 
  • #46
wabbit said:
You'd need to be in its remote suburbs though, otherwise I suspect the sky would be so bright from all the nearby stars surrounding you that you wouldn't see the milky way at all. Which would be quite a sight in its own right...
even if you are in remote suburbs you will be able to see the MW only for half of the year . can you see how ? :smile:
 
  • #47
vrmuth said:
even if you are in remote suburbs you will be able to see the MW only for half of the year . can you see how ? :smile:
Oh it's even worse than that : you also need your star to be on the right part of its orbit around the center of the cluster lest the cluster blocks the view. Lots of geometric constraints to combine...
 
  • #48
The Senior Editor of Astronomy Magazine, Michael E. Bakich, has given approval for us to post the article, "Life Inside a Globular Cluster", written by William E. Harris and Jeremy Webb, from the July 2014 issue, on Physics Forums. See the attached pdf.

I wish to thank Michael E. Bakich, and Astronomy Magazine, for this gracious gift to the members of Physics Forums!

Please thank Astronomy Magazine by liking this post, or better yet, giving a gift subscription to a friend, or even yourself. (I am fully responsible for that plug)
 

Attachments

  • Like
Likes   Reactions: Garth, Greg Bernhardt, vrmuth and 2 others
  • #49
I recently spotted this arXiv article, and it fits this post well.

Two stellar-mass black holes in the globular cluster M22
The paper made it into http://www.nature.com/nature/journal/v490/n7418/full/nature11490.html.

I'd not seen it before, but the Milky Way globular cluster, M22, apparently has at least TWO black holes. From the abstract:
"...we report the presence of two flat-spectrum radio sources in the Milky Way globular cluster M22, and we argue that these objects are black holes of stellar mass (each ∼ 10–20 times more massive than the Sun) that are accreting matter." and M22 may contain a total population of ∼ 5–100 black holes."

Here are a few interesting extracts from the arXiv paper:
1. ...the objects cannot be black-hole/black-hole binaries, and instead are probably in binary systems with Roche lobe-overflowing companions
[ for an explanation of the Roche Lobe, see ]

2. Stellar-mass black holes will mass-segregate to the core of the cluster.

3. The presence of black holes in a globular cluster can lead to an expansion of the core radius through interactions between black holes and stars. This could explain why M22 has the fifth largest core radius among luminous ( >∼ 2 × 105L ) Milky Way globular clusters

M22.png
 
Last edited by a moderator:
  • #50
IMO, globular clusters probably preceded ordinary galaxies in the universe. I suspect most of them harbor black holes of significant mass. There is observational evidence favoring this idea, which also explains why they tend to be populated by ancient stars.
 
  • #51
Black holes in globular clusters appear to be rare, or at least, mostly undiscovered. This quote, "In 2007, Maccarone made the first discovery of a black hole in a globular star cluster in the neighboring NGC4472 galaxy." from PHYSICISTS FIND BLACK HOLES IN GLOBULAR STAR CLUSTERS, UPSETTING 40 YEARS OF THEORY shows how recent the discovery of black holes in globular clusters actually is. I think only a few GCs are currently known to harbor black holes. And if you look at the image above, showing the location of the two BHs, you'll see that they are not actually in the center, but near it, which might be more of a reflection on statistics than an 'evolution of globular cluster' occurrence.

What struck me about the paper was that there appear to be many black holes in this one GC. As it stands now, there are only a few GC known to have black holes. And new to me was the idea that the black holes get ejected. If so, there should be renegade black holes flying through space.
 

Similar threads

Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 12 ·
Replies
12
Views
4K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K