Institute of research into the fundamental laws of the Universe

A burst of star formation in a galaxy of the distant Universe

When the Universe was only 3 billion years old, galaxies had very different properties than those they exhibit nowadays. Their shapes were more irregular and their disks were much more gas-rich. We actually know that the latter formed their stars more rapidly, within gigantic, much more massive and luminous star-forming regions than those typically observed in local galaxies. However, the way these large stellar clumps formed is not yet understood, and their evolution along cosmic history is still highly debated. To clarify these open issues, astrophysicists from SAp carried out their own observing campaign with the Hubble Space Telescope (in imaging and spectroscopic mode) and the Subaru Telescope (in spectroscopic mode) installed in Hawaii. Indeed, the apparent faintness of distant galaxies requires the use of powerful observing facilities. They discovered the signature of a giant clump made of very young stars and caught while just forming, within a galaxy located at a distance of 11 billion light-years.
Less than 10 Million years old, this clump has not yet evolved enough for its stars to be directly detected. Therefore it is thanks to the radiations from the gas ionized by these young stars that it was revealed. This giant clump has a gas mass of about one billion times that of the Sun. Forming its stars at a rate of 30 solar masses per year, it contributes up to 50% of the total star formation of the galaxy. Besides, its growth rate in mass and its efficiency in converting molecular gas into new stars are 10 times higher than the typical values observed at this epoch of cosmic history. This confirms the presence of a prodigious burst of star formation in this region.

Numerical simulations at very high resolution

To supplement the interpretation of these unprecedented results, the scientists also developed a set of hydro-dynamical simulations at very high resolution using the super computer of the « Très Grand Centre de Calcul » of CEA and GENCI. These simulations show that in gas-rich galaxies, gravitational instabilities and turbulence within the interstellar medium lead the gas to fragment and collapse, which then results in the birth of a host of new stars, concentrated in regions which size can reach several hundred light-years. Within these stellar clumps, the instantaneous star-forming activity undergoes dramatic increase during the very first few million years, to reach values remarkably close to that inferred from the observations obtained by Zanella and her team. The star forming efficiency in these regions is also larger than the typical value measured at galaxy scales. Then, after about 15 million years, the feedback and stellar winds from the young massive stars and the explosion of the first supernovae become strong enough to counterbalance the gravitational collapse of the gas. Star formation hence gradually declines, while still maintaining an efficiency higher than that characterizing the other disk regions.

A possible mechanism to explain the growth of galaxy bulges

The discovery of such a young star-forming region in a distant galaxy has crucial implications on the understanding of galaxy formation at cosmological scale. The young and massive clump discovered by the researchers of CEA reveals indeed rare physical properties, only observable during the ~15 million years following the gravitational collapse of the gas and the birth of such concentrations of new stars. Among the ~60 galaxies observed as part of this study, it is actually the only object showing such characteristics. Giant clumps found in the other distant galaxies correspond indeed to much more evolved stellar regions. Hence, the scarcity of the phenomenon discovered here implies that the lifetime of the clumps observed in the distant Universe could reach at least 500 million years. This new constraint excludes theoretical scenarios that predict their rapid destruction by the feedback and the action of the winds originating from newly-formed stars, and it corroborates the idea that these giant clumps can survive long enough to evolve within the galactic disk where they were born. They could then migrate toward the core of the galaxy and play a major role in the growth of the bulge and the central super-massive black hole.

Properly characterizing the role of these giant clumps in galaxy evolution will yet require an even more accurate determination of their physical properties, such as their size and dynamical mass. Increasing the statistical sample of such young star-forming regions will also be a central part of the forthcoming work led by the research group. Such studies will require in particular the use of observing facilities like the ALMA (Atacama Large Millimeter Array) network of radio antennae installed in northern Chile, as well as the James Webb Space Telescope (JWST) whose launch is planned for the end of 2018.

Contacts : Anita Zanella, Emeric Le Floc'h

Publication :

"An extremely young massive clump forming by gravitational collapse in a primordial galaxy"
A. Zanella, E.Daddi, E. Le Floc’h, F. Bournaud, R.Gobat, F. Valentino, V. Strazzullo, A. Cibinel, M. Onodera, V. Perret, F. Renaud, C. Vignali
published in the Nature journal, May 2015
Access to the  electronic version of the publication

See also          - The CEA press release  (7 may 2015)

Voir aussi : Comment nourrir les trous noirs géants ? (11 novembre 2011, in french)
                 Les clés de l'évolution des galaxies (Point Presse - 7 juin 2013 - in french)

Written by : Emeric Le Floc'h, C. Gouiffès