Science Forums: GRBs from collapse of NSCs --> SMBHs ?? - Science Forums

Jump to content

Welcome to ScienceForums.Net!

Welcome to ScienceForums.Net! We welcome science discussion at all levels — from beginners to researchers, covering topics from biology to computer science, and much more. Registration is fast and free, and allows you to post on the forums, so register now and join the discussions!
  
After you've registered, come in and introduce yourself, or visit the forum index. If you need any help  registering, posting, or if you just have some questions about our site, please feel free to contact us at staff at scienceforums dot net.

  • Start new topics and reply to others
  • Subscribe to topics and forums to get automatic updates
  • Create a ScienceForums.Net Blog!
Guest Message © 2012 DevFuse
Page 1 of 1
  • You cannot start a new topic
  • You cannot reply to this topic

GRBs from collapse of NSCs --> SMBHs ?? 'wet' mergers of proto-galaxies => SMBHs, GRBs ? Rate Topic: -----

#1 Widdekind 


Atom
Nuclear Star Clusters resemble massive Globular Clusters, residing in the cores of small galaxies (Ho. Galaxy Formation & Evolution). NSCs, in low-mass galaxies, are associated with surface-brightness 'cusps', having 'disky' isophotes, and evidencing weak rotation. High-mass galaxies tend to host SMBHs, instead of NSCs (Mason. Astrophysics Update 2, p.180). According to 'Hierarchical Structure Formation', small proto-galaxies merge, to make larger galaxies. And, in 'wet' gas-rich galaxy mergers, gas gets 'funneled' to the center of the system, whereat NSCs would reside. Perhaps, then, when small, gas-rich proto-galaxies merge, gas gets funneled to the center, enveloping all the stars in a 'common envelope', which absorbs stellar energies & angular momenta, leading to a 'collapse' of the NSCs into SMBHs ?? If so, could the catastrophic collapses, of millions of stars, into SMBH, generate GRBs ??

Posted Image
'wet', i.e. gas-rich, proto-galaxy core

Posted Image
GRB in core of galaxy

0

#2 Widdekind 


Atom
Observation, of a 2 billion solar-mass SMBH, when our universe was <1 Gyr old, apparently precludes the possibility, that this SMBH formed from the merger of star-mass BHs. Instead, a large-scale "direct collapse" appears more plausible (Science News 2011).
0

#3 Airbrush 


Molecule
Interesting observation. I had always believed SMBH formed long before any stars or galaxies. The only way that much matter can be close enough together is soon after the moment of the Big Bang.

This post has been edited by Airbrush: 12 December 2011 - 09:22 PM

When in doubt, Wiki it out.

How do you dodge a bullet on your way to another star while traveling 12%C?
0

#4 Widdekind 


Atom

View PostAirbrush, on 12 December 2011 - 09:21 PM, said:

Interesting observation. I had always believed SMBH formed long before any stars or galaxies. The only way that much matter can be close enough together is soon after the moment of the Big Bang.


I'm arguing for a sudden-and-catastrophic "implosion", of an entire cluster, of millions of stars, "mired" amidst a "common envelope" of gas & dust that "saps" their orbital energies, until they all "sink" towards their system center, "past the point where the space-time fabric can support their mutual mass", so that "the rubber trampoline mat sags & rips", suddenly forming an entire SMBH, in situ, all at once.
0

#5 Arch2008 


Baryon
Maybe not...

http://www.dailygala...r-big-bang.html

http://www.astronomy...al&utm_content=

http://www.scienceda...11212124557.htm

I haven't found the paper in Arxiv...yet.

Here you go:
http://arxiv.org/abs/1107.1253

This post has been edited by Arch2008: 16 December 2011 - 05:35 PM

B.S. never has room enough in a fact or a truth, but it always fits perfectly into an opinion.
1

#6 Widdekind 


Atom
Thanks for the links... they discuss how the first SMBH grew (and, grew quickly); yet, I was asking, about how they formed (collapse of large star clusters??):

Quote

the very first black holes, those that started the entire growth process when the universe was only several hundred million years old, had masses of only 100-1000 times the mass of the sun. Such black holes may be related to the very first stars in the universe [i.e. (cores of dense) star clusters]. They also found that the subsequent growth period of the observed sources...lasted only 100-200 million years [cp. characteristic life-time of quasars is 100-200 Myr] (science daily 2010).

More than half of detected SMBH are heavily obscured, in enshrouding dust & debris, "black holes must be hidden behind large quantities of dust and gas from their host galaxies" (science daily 2011, science daily 2011). That is what a "wet collapse" scenario would resemble.

This post has been edited by Widdekind: 24 December 2011 - 12:23 AM

0

Share this topic:


Page 1 of 1
  • You cannot start a new topic
  • You cannot reply to this topic

1 User(s) are reading this topic
0 members, 1 guests, 0 anonymous users