Amazing image shows a dying galaxy ejecting 10,000 Suns-worth of gas every year after a giant collision - weakening its ability to form stars

A sensational image of a dying galaxy - ejecting 10,000 Suns-worth of gas every year due to a large collision - has been captured by an international team of astrono-mers.

New research led by Durham University  looked  nine  billion years into the past in search of evidence that galaxy mergers in the early universe could stop star formation.

These mergers force gas to leak from the galaxy and weaken its ability to form new stars, effectively marking the end of its life as an active body.  

The team found that a huge amount of star-forming gas was ejected into the intergalactic medi-um by the coming together of two galaxies.

Researchers say that this event, together with a large amount of star formation in the nuclear regions of the newly merged galaxy - dubbed ID2299 - will eventually deprive the single merged body of the fuel needed for new stars to form.  This would stop star formation for several hundred million years, effectively halting the galaxy's development.

Due to the amount of time it takes the light from ID2299 to reach Earth, the researchers were able to see the galaxy as it would have appeared nine billion years ago when it was in the late stages of its merger.

This is a time when the universe was only 4.5 billion years old and was in its most active, 'young adult' phase - if compared to a human life.Using the European Southern Observatory's  Atacama  Large Millimeter  Array (ALMA) teles-cope in northern Chile, the resear-chers saw it was ejecting about half of its total gas reservoir into the galaxy surroundings at a rate equivalent to 10,000-Suns worth of gas each year.

Lead  author  Dr Annagrazia Puglisi, in Durham University's Centre for Extragalactic Astro-

nomy, said: 'We don't yet know what the exact processes are be-hind the switching off of star for-mation in massive galaxies.'Feedback driven winds from star formation or active black holes are thought to be the main respon-sible for expelling the gas and quenching the growth.

'Our research provides evidence that the gas being flung from ID2299 is likely to have been tidally ejected because of the merger between two gas rich galaxies. 'The gravitational interaction bet-ween two galaxies can thus provide sufficient angular momentum to kick out part of the gas into the galaxy surroundings.

'This suggests that mergers are also capable of altering the future evolution of a galaxy by limiting its ability to form stars over millions of years and deserve more inves-tigation when thinking about the factors that limit galaxy growth.'

Researchers were able to rule out star formation and the galaxy's active black hole as the reason for this ejection by comparing their measurements to previous studies and simulations and by measuring the physical properties of the escaped gas.

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

Researchers say that simulations suggest that no black holes can kick out as much cold gas from a galaxy as seen expelled from ID2299.

The excitation of the escaped gas is also not compatible with a wind generated by a black hole or the birth of new stars.

Co-author Dr Emanuele Daddi, from CEA-Saclay said: 'This galaxy is witnessing a truly extreme event.'It is probably caught during an important physical phase for galaxy evolution that occurs within a relatively short time window. We had to look at over 100 galaxies with ALMA to find it.'

Fellow co-author Dr Jeremy Fensch, of the Centre de Recherche-Astrophysique de Lyon, added: 'Studying this single case unveiled the possibility that this type of event might not be unusual at all and that many galaxies suffered from this 'gravitational gas removal', in-cluding misinterpreted past obser-vations.

'This might have huge conse-quences on our understanding of what actually shapes the evolution of galaxies.'The researchers now hope to obtain higher resolution images of ID2299 and other distant galaxy mergers and carry out computer simulations to further understand the effect galaxy mergers have on the life cycle of galaxies.

The findings are published in the journal Nature Astronomy. WHAT IS ALMA?Deep in the Chilean desert, the Atacama Large Millimetre Array, or ALMA, is located in one of the driest places on Earth.At  an altitude  of  16,400 ft, roughly half the cruising height of a jumbo jet and almost four times the height of Ben Nevis, workers had to carry oxygen tanks to com-plete its construction.Switched on in March 2013, it is the world's most powerful ground based telescope.It is also the highest on the planet and, at almost £ - 1 billion ($ -1.2 billion), one of the most expensive of its kind.