The project, coordinated by the Andalusian Institute of Astrophysics, has allowed unravelling the history of star formation in the galactic centre, with a huge sample of them
The Galacticnucleus project, coordinated by researchers from the Institute of Astrophysics of Andalusia (IAA-CSIC), was designed to study the central region of the Milky Way, which represents the most extreme astronomical environment we can study in detail, with a supermassive black hole surrounded of a dense star cluster.
With a sample of stars one hundred times higher than in previous projects, Galacticnucleus has allowed to unravel the history of star formation in the galactic center and detect what was possibly its most energetic episode, a burst of star formation that produced more than one hundred thousand Supernova explosions
“For the first time we have obtained a detailed vision of the process of star formation in a large region of the galactic centre,” says the astronomer of the IAA-CSIC and coordinator of the Galacticnucleus project, Rainer Schödel. “Contrary to what was expected, we have discovered that the formation of stars has not been continuous,” says Francisco Nogueras-Lara, a researcher at the IAA-CSIC and first author of the study, published in ‘Nature Astronomy’.
The study reveals that about 80% of the stars in the center of the Milky Way were formed in the remote past, between eight and thirteen billion years ago. This period of initial star formation was followed by some six billion years of latency during which stars were barely born. This sterile period came to an end with an intense burst of star formation about a billion years ago: stars with a combined mass of several tens of millions of suns formed in the galactic center in a period of less than one hundred million years.
“The conditions in the galactic center during this burst of activity must have resembled those of the ‘starburst’ galaxies – literally starbursts – which show a rate of star formation of more than one hundred solar masses per year, much higher than the current rate of the Milky Way, which oscillates annually between one and two solar masses, “notes Nogueras-Lara, who is now researching at the Max Planck Institute for Astronomy in Heidelberg (Germany).
Violent Supernova Explosions
In this type of starburst, many massive stars are born, which have a short life: they burn their fuel, nuclear hydrogen, much faster than lower mass stars and culminate their lives with violent supernova explosions. “This outbreak of activity, which resulted in the explosion of more than one hundred thousand supernovae, was probably one of the most energetic events in the entire history of the Milky Way,” concludes Rainer Schödel (IAA-CSIC).
This outbreak was followed by a period of reduced activity, but in the last tens of millions of years the galactic center has been forming stars at a relatively high rate. This result changes our image of how stars are formed in the central region of the Milky Way and “instead of a constant star formation, this part of the galaxy has notorious peaks of activity throughout its history.”
Thanks to an infrared camera
This research was made possible by the observations of the galactic center made with the HAWK-I instrument of the VLT telescope (ESO) in the Atacama desert (Chile). This infrared camera, capable of seeing through the dust clouds of the galactic center, made it possible to obtain the most detailed image of the galactic center, published in October. For this, more than three million stars were studied, covering an area corresponding to more than sixty thousand square light-years.
Studying the center of the Milky Way is essential to obtain a complete picture of how our galaxy formed. The data obtained under the Galacticnucleus project also allow a better understanding of the structure and properties of the galactic center, as well as its stellar populations.