The largest explosion ever seen in space

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Discussion Overview

The discussion centers around the recent discovery of the largest explosion ever observed in space, which has implications for understanding the role of supermassive black holes (SMBH) in galaxy formation and evolution. Participants explore the potential effects of black holes on star formation and the cooling flow model in galaxy clusters, as well as the observational challenges in studying early galaxy formation.

Discussion Character

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

Main Points Raised

  • Some participants highlight that the explosion suggests black holes may inhibit star formation by creating regions of hot gas that prevent condensation.
  • Others propose that there is an optimal amount of black hole mass that promotes star formation, indicating a complex relationship between black holes and galaxy evolution.
  • A participant mentions that the cooling flow model problems in galaxy clusters may be addressed by these findings, suggesting that jets from black holes heat the gas and reduce star formation.
  • Some express interest in the observational limitations regarding early galaxy formation and the difficulties in characterizing selection effects in distant objects.
  • There are mentions of ongoing research related to merging clusters of galaxies and the environments of starburst galaxies, indicating a variety of research interests among participants.
  • Participants share links to related articles and preprints, indicating a collaborative effort to explore the topic further.

Areas of Agreement / Disagreement

Participants express a range of views on the implications of the discovery, with no clear consensus on the exact role of black holes in star formation or the validity of the cooling flow model. The discussion remains unresolved with multiple competing perspectives presented.

Contextual Notes

Participants note that the observational techniques available may limit understanding of early galaxy formation, and there are unresolved questions regarding the cooling flow model and the density of gas in galaxy clusters.

Who May Find This Useful

Readers interested in astrophysics, particularly in the areas of galaxy formation, black hole dynamics, and observational astronomy may find this discussion relevant.

Chronos
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Hot off the press:
http://www.space.com/scienceastronomy/big_explosion_050105.html

The largest explosion ever seen in space reveals black holes to be more influential than expected, perhaps sometimes stifling star formation in a galaxy while gobbling up trillions upon trillions of tons of gas.
Another potential piece in the puzzle of galactic evolution. There is a link to another less recent article discussing SMBH influences on galactic formation.
 
Astronomy news on Phys.org
Wow, Paul Nulsen is one of my PhD supervisors! Go the Aussies!

These results may also help to solve the cooling flow model problems in clusters of galaxies.
 
matt.o said:
Wow, Paul Nulsen is one of my PhD supervisors! Go the Aussies!

These results may also help to solve the cooling flow model problems in clusters of galaxies.

Congratulations to him on the discovery. and to Brian McNamara and the rest. it said the thing is written up in 6 january 2005 Nature, maybe we can find an online preprint

I would be interested to learn what your research is about, matt.o, if you'd care to say.

this news item presents an "optimality problem" in a curious way
there seems to be a RIGHT AMOUNT of black hole to promote starformation

BHs play an important role in the formation of galaxies (isnt that current thinking?) but this discovery illustrates that TOO MUCH BH interferes with star formation and causes large "bubbles" (on order of a million LY diameter) where no stars form because I guess the gas there is too hot to condense.

I admit to idle speculation here and will hold off any further for the moment
 
The formation of galaxies, SMBH, even the first (few) generation(s) of stars are hot topics in astronomy. Unfortunately, the era at which this (first) took place is only barely accessible to current observational instruments and techniques, so one is always left with the nagging doubt about what the few observations of these distant (or old) objects actually tell us; for example, selection effects are particularly difficult to characterise.

(note that MS 0735.6+7421 - at ~3 billion ly - is neither distant nor old, wrt the 'first formation' era).

I'll leave others to comment on the current theoretical thinking.
 
100 millions years of eruption. Wow, that's pretty amazing.
 
marcus said:
Congratulations to him on the discovery. and to Brian McNamara and the rest. it said the thing is written up in 6 january 2005 Nature, maybe we can find an online preprint

I would be interested to learn what your research is about, matt.o, if you'd care to say.

this news item presents an "optimality problem" in a curious way
there seems to be a RIGHT AMOUNT of black hole to promote starformation

BHs play an important role in the formation of galaxies (isnt that current thinking?) but this discovery illustrates that TOO MUCH BH interferes with star formation and causes large "bubbles" (on order of a million LY diameter) where no stars form because I guess the gas there is too hot to condense.

I admit to idle speculation here and will hold off any further for the moment


I have the article from nature, will link here soon.

For some idle speculation, let's go-ogle at these:https://www.physicsforums.com/showthread.php?t=39328

A number of posts here:Number six!..: https://www.physicsforums.com/showthread.php?p=140213#post140213

and of course under an 'alias' poster here:https://www.physicsforums.com/showthread.php?t=24178

Unlucky for some #13:https://www.physicsforums.com/showthread.php?t=35367&page=1&pp=15

The list goes on!..the outcome if proven will be far reaching.

I admit to speculate.
 
Last edited:
Here are some excellent images and animations of MS 0735. To get some idea of how big these cavities are, there’s a comparison to the cavities in the Perseus cluster which is only 250 million light years away.
 
here is the arxiv preprint link for the nature paper:

http://arxiv.org/abs/astro-ph/0411553

marcus:

my PhD involves studying merging clusters of galaxies in multiple wavelenghts, cold fronts within clusters of galaxies, evolution of galaxies in a clustered environment and probably some modelling of merging clusters (eventually). At the moment I am using 2dfgrs data to study the environments of starburst galaxies.

BHs play an important role in the formation of galaxies (isnt that current thinking?) but this discovery illustrates that TOO MUCH BH interferes with star formation and causes large "bubbles" (on order of a million LY diameter) where no stars form because I guess the gas there is too hot to condense.

the general consensus was that in relaxed clusters a cooling flow develops. this causes gas to cool and flow to the centre of the cluster. it was thought that this gas would flow to the bottom of the potential well (the cD galaxy at the centre) and condense enough such that star formation could take place. The problem was, there was never enough cool gas observed in these cD's compared to what the cooling flow models predicted. So these jets serve to heat up the gas that permeates the central parts of the cluster and stops the cooling flow for a period of time. This means there will be less gas than expected cooling out of the x-ray temp range. So this means we will see less cool gas than predited from cooling flow models, hence less star formation in the cD than expected.

you are right, the x-ray emitting gas is too hot to condense and form stars, but is also far from dense enough. the densest parts of the intra cluster medium are less dense than any vacuum we can create on earth!


DB:

100 million years is but a blink of an eye to these monsters. processes in clusters generally take billions of years to complete!

matt.
 
Brian McNamara is my advisor here at OU...he's actually teaching my Astro class right now. I got to see him present the finding at the AAS conference a few weeks back. THAT was a cool trip.
 

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