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STELLAR CHEMISTRY
Galaxy mergers could limit star formation
by Staff Writers
Durham UK (SPX) Jan 12, 2021

illustration only

Our astronomers have looked nine billion years into the past to find evidence that galaxy mergers in the early universe could shut down star formation and affect galaxy growth.

Using a powerful Earth-based telescope they saw that a huge amount of star-forming gas was ejected into the universe by the coming together of two galaxies.

The merger created a new galaxy called ID2299 at a time when the universe was only 4.5 billion years old.

The researchers say that this event, combined with huge star formation in the galaxy's nuclear regions, could eventually deprive it of the fuel needed to make stars.

This would stop star formation for several hundred million years, effectively halting the galaxy's development.

Active black holes
Astronomers observe many massive, dead galaxies containing very old stars in the nearby Universe and don't exactly know how these galaxies have been formed.

Simulations suggest that winds generated by active black holes as they feed, or those created by intense star formation, are responsible for such deaths by expelling the gas from galaxies.

Now our new study offers galaxy mergers as another way of shutting down star formation and altering galaxy growth.

Observational features of winds and "tidal tails" caused by the gravitational interaction between galaxies in such mergers can be very similar.

Galactic winds
But the rate at which the gas is being expelled from ID2299 is too high to have been caused by the energy created by a black hole or starburst as seen in previous studies.

Computer simulations also suggest that black holes can't kick out as much cold gas from a galaxy as seen in this study.

Therefore, researchers suggest that some past results where galactic winds have been seen as the cause of halting star formation might need to be re-evaluated.

Research paper


Related Links
Durham University
Stellar Chemistry, The Universe And All Within It


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Washington DC (UPI) Jan 7, 2021
The brown dwarf closest to our solar system hosts wind bands and jet streams, according to new analysis of the object's atmosphere. Brown dwarfs are too big to be planets but not quite massive enough to generate fusion, a prerequisite for stellar classification. Though hot in their infancy, brown dwarfs steadily cool as they mature, making them difficult to spot and study. Because they don't generate their own light, imaging the atmosphere of a brown dwarf is difficult. Little is known a ... read more

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