They may only be little, but they pack a star-forming punch: new observations from the NASA/ESA Hubble Space Telescope show that starbursts in dwarf galaxies played a bigger role than expected in the early history of the Universe.
Although galaxies across the Universe are still forming new stars, the majority of the stars were formed between two and six billion years after the Big Bang. Studying this early epoch of the Universe’s history is key in order to fully understand how these stars formed, and how galaxies have grown and evolved since.
A new study using data from Hubble’s Wide Field Camera 3 (http://www.spacetelescope.org/about/general/instruments/wfc3/) (WFC3) has allowed astronomers to take a new step forward in understanding this crucial era by peering at a sample of dwarf galaxies in the early Universe and, in particular, a selection of starburst galaxies within this sample. These starburst galaxies form stars at a furiously fast rate, far above the “normal” star formation rate expected of galaxies. Previous studies of starburst galaxies have focussed on analysing mid-range or high-mass galaxies, leaving out the huge number of dwarf galaxies that existed in this era of prolific star formation.
It was not previously possible to study these distant small galaxies closely. Astronomers could only observe small galaxies at smaller distances or larger galaxies at greater distances. The highly sensitive infrared capabilities of WFC3 and its unique grism spectroscopy mode  have now allowed astronomers to peer at low-mass dwarf galaxies in the distant Universe and to deduce the contribution of the starburst galaxies to the total star formation within dwarf galaxies at that time.
“We already suspected that dwarf starbursting galaxies would contribute to the early wave of star formation, but this is the first time we’ve been able to measure the effect they actually had,” says Hakim Atek of the École Polytechnique Federale de Lausanne (EPFL) in Switzerland, lead author of the new paper. “They appear to have had a surprisingly significant role to play during the epoch where the Universe formed most of its stars.”
“These galaxies are forming stars so quickly that they could actually double their entire mass of stars in only 150 million years — This sort of gain in stellar mass would take most normal galaxies 1-3 billion years,” adds co- author Jean-Paul Kneib, also of EPFL.
This result contributes to a decade-long investigation to understand the links between galaxies’ mass and their star-forming activity, and helps to paint a consistent picture of events in the early Universe.
As well as adding new insight into how and where the stars in our Universe formed, this new finding will certainly help to unravel the secrets of galactic evolution. It is unusual to find a galaxy in a state of starburst, implying that they are the result of some strange incident, such as a merger, a tidal interaction with another galaxy, or the shockwave from a supernova. By studying these galaxies more closely and understanding how they formed and behaved in their earliest years, astronomers hope to discover the cause of these violent bursts and learn more about galactic evolution throughout the Universe.
 The grism splits up the light from the galaxies, revealing the distribution of brightness and colour in the Universe. This allows scientists to deduce facts about their chemical composition and distance from Earth that would not be possible without such a detailed view from Hubble’s space-based perspective.
Notes for editors:
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.
 The international team of astronomers in this study consists of Hakim Atek (EPFL, Switzerland); Jean-Paul Kneib (EPFL, Switzerland); Camilla Pacifici (Yonsei University Observatory, Republic of Korea); Matthew Malkan (University of California, USA); Stephane Charlot (Institut d’Astrophysique de Paris,France); Janice Lee(Space Telescope Science Institute,USA); Alejandro Bedregal ( Minnesota Institute for Astrophysics, USA); Andrew J. Bunker (University of Oxford, UK); James W. Colbert (Spitzer Science Center, USA); Alan Dressler (Observatories of the Carnegie Institution for Science, USA); Nimish Hathi(Aix Marseille University, France); Matthew Lehnert (Institut d’Astrophysique de Paris, France); Crystal L. Martin (Dep’t. of Physics, Univ. of Calif, USA); Patrick McCarthy (Observatories of the Carnegie Institution for Science, USA); and Marc Rafelski (Spitzer Science Center, USA); Nathaniel Ross (University of California, USA); Brian Siana (University of California Riverside, USA); and Harry I. Teplitz (Caltech, USA)
Hakim Atek, Tel: +41 78 722 9026, Email: firstname.lastname@example.org
Jean-Paul Kneib, Tel: +41 22 3792473, Cell: +33 695 795 392, Email: email@example.com
Georgia Bladon, Tel: +49-89-3200-6855, Email: firstname.lastname@example.org