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Globular Clusters are swallowed Galaxies


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Computer Simulations suggest that:

hundreds of medium-sized
Black Holes
are roaming loose in the
Milky Way
. These rogues... are the
orphaned
Central Black Holes
of the many smaller
Galaxies
that the
Milky Way
has swallowed
over its
billions of years
of existence.

For:

Galaxies
, such as our own, most often grow by absorbing smaller, satellite galaxies, such as the
Large Magellanic Cloud
, which orbits the
Milky Way
.

And:

each of the hundreds of billions of
Galaxies
in the
Cosmos
formed a massive or supermassive
Black Hole
at its center [and] when big
Galaxies
collide -- a relatively common occurrence -- their central
Black Holes
eventually merge.

But:

sometimes the central
Black Hole
of a
Dwarf Galaxy
might remain independent after a
Galactic Collision
... The ejected
Black Hole
would not move fast enough to escape the
Galaxy's
gravity entirely
, but it would move faster than the background stars--something that makes it detectable, because it would also be dragging along a
small cluster of surrounding stars
... the researchers suggest searching the galaxy for compact and relatively fast-moving
clusters of old stars
*
.

Now, "compact clusters of old stars" sounds suspiciously like Globular Clusters:

supermassive
Globular Clusters
are in fact the cores of
Dwarf Galaxies
that are consumed by the larger
Galaxies
.
Several
Globular Clusters
(like
M15
[in our
Milky Way Galaxy
,
33.6 thousand light-years away
, in
Pegasus Constellation
]
)
have extremely massive Cores which may harbor
Black Holes
...

 

a
4,000 Solar-mass
Intermediate-mass Black Hole
has been suggested to exist
, based on HST
[
Hubble Space Telescope
]
observations,
in the
Globular Cluster
M15
, and a
20,000 Solar-mass
Black Hole
in the
Mayall II
cluster in the
Andromeda Galaxy
. Both x-ray and radio emissions from Mayall II appear to be consistent with an intermediate-mass black hole.

 

These are of particular interest because they are the first black holes discovered that were intermediate in mass between the conventional stellar-mass
Black Hole
and the supermassive
Black Holes
discovered at the cores of
Galaxies
.
The mass of these
Intermediate-mass Black Holes
is proportional to the mass of the clusters, following a pattern previously discovered between
Supermassive Black Holes
and their surrounding
Galaxies
**
.

This strongly suggests, that Globular Clusters are ancient Dwarf Galaxies, having "Dwarf Black Holes" at their cores.

*

**

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  • 2 weeks later...

Nice info Widdekind, thanks for sharing. I understood you 100% this time. Let's be on the lookout for an entourage of stars following a medium massive black hole thru our galaxy.

 

How do you think supermassive black holes originally formed? I seems to me they must have formed at the time of the big bang because how does that much matter, Millions or Billions of solar masses, get close enough together to create a SBH? Stars are too disbursed and have too much motion to all fall together like that.

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I read somewhere that gas falling into the center of the galaxy would form a gas disk and would have to lose 99.9% of its angular momentum before it could even get close to the black hole.

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That is what I mean granpa, there was too much angular momentum, and low density so very little gravity in the swirling expanding masses of gas and dust, for it to all just fall into the middle and become a SBH. The original eddys in the early big bang became SBHs.

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Perhaps the Big Bang was the Explosive Evaporation of a "Hyper-Massive Black Hole":

Perhaps your SMBHs are "chunks" of BH material blown outwards by that explosion, akin to knots of gas blown out by Supernovae. Those "BH fragments" then formed the seeds of Galaxies w/in our Universe -- to wit, inside the expanding "Explosion Remnant" (akin to Supernova Remnants).

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