Astronomers use Hubble to study bursts of star formation in the dwarf galaxies of the early Universe

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 (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 [1] 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 Fédérale 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

[1] 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.

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, Suisse) ; Jean-Paul Kneib (directeur de recherche au CNRS détaché à l'EPFL, Suisse) ; Camilla Pacifici (Yonsei University Observatory, République de Corée) ; Matthew Malkan (University of California, USA) ; Stéphane Charlot (Institut d'Astrophysique de Paris-CNRS-UPMC, 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 (Université d'Aix Marseille, France) ; Matthew Lehnert (Institut d'Astrophysique de Paris-CNRS-UPMC, France) ; Crystal L. Martin (Dep't. of Physics, Univ. of Calif, USA) ; Patrick McCarthy (Observatories of the Carnegie Institution for Science, USA) ; Marc Rafelski (Spitzer Science Center, USA) ; Nathaniel Ross (University of California, USA) ; Brian Siana (University of California Riverside, USA) ; et Harry I. Teplitz (Caltech, USA)

ESA Press Release


NASA Press Release

Astrophysical Journal : "Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts Across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe" and arXiv/Astro-ph

Hakim Atek
École Polytechnique Fédérale de Lausanne, Sauverny, Switzerland.
hakim.atek at epfl.ch
Tél. : +41 78 722 9026

Jean-Paul Kneib
École Polytechnique Fédérale de Lausanne, Sauverny, Switzerland
jean-paul.kneib at epfl.ch
Tél. : +41 22 3792473
Mobile : +33 695 795 392

Stéphane Charlot
Institut d'Astrophysique de Paris-CNRS-UPMC
charlot at iap.fr
Tél. : +33 1 4432 8183

Georgia Bladon
ESA/Hubble, Public Information Officer, Garching, Germany
gbladon at partner.eso.org
Tél. : +49-89-3200-6855

Image A : le champ GOODS contenant les galaxies naines distantes

GOODS field containing distant dwarf galaxies forming stars at an incredible rate (annotated)

This image shows the area containing a sample of dwarf galaxies studied to unlock secrets of star formation in the early Universe. Highlighted are faint dwarf galaxies that reside in the early Universe, between two and six billion years after the Big Bang, an important time period when most of the stars in the Universe were formed. Some of these galaxies are undergoing starbursts and have been studied by astronomers to deduce their contribution to star formation in this crucial era of the Universe's history. The image is part of the Great Observatories Origins Deep Survey (GOODS), and this image shows only one section that the survey covered.

Image C : illustration représentant une image grism de Hubble

Concept illustration of a grism image

This image represents the data that comes from using the NASA/ESA Hubble Space Telescop's highly-sensitive Wide Field Camera 3 in its grism spectroscopy mode. A grism is a combination of a grating and a prism, and it splits up the light from a galaxy into its constituent colours, producing a spectrum. In this image the continuum of each galaxy is shown as a "rainbow". Astronomers can look at a galaxy's spectrum and identify light emitted by the hydrogen gas in the galaxy. If there are stars being formed in the galaxy then the intense radiation from the newborn stars heats up the hydrogen gas and makes it glow. All of the light from the hydrogen gas is emitted in a small number of very narrow and bright emission lines. For dwarf galaxies in the early Universe, the emission lines are much easier to detect than the faint, almost invisible, continuum originating from stars, the only light present between the hydrogen emission lines.

Crédits images : NASA, ESA, H. Atek (EPFL, Suisse) and J-P. Kneib (EPFL, Suisse)

June 2014

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