A Chalmers-led team of scientists has studied two galaxies in the early universe, which contain extremely productive star factories. Using powerful telescopes to split the galaxies’ light into individual colours, the scientists were amazed to discover light from many different molecules – more than ever before at such distances. Studies like this could revolutionize our understanding of the lives of the most active galaxies when the universe was young, the researchers believe.
When the universe was young, galaxies were very different from today’s stately spirals full of gently-shining suns and colourful gas clouds. New stars were being born, at rates hundreds of times faster than in today’s universe. Most of this however, was hidden behind thick layers of dust, making it a challenge for scientists to discover these star factories’ secrets, until now.
By studying the most distant galaxies visible with powerful telescopes, astronomers can get glimpses of how these factories managed to create so many stars.
In a new study, published in the journal Astronomy & Astrophysics, a team of scientists led by Chalmers astronomer Chentao Yang, used the telescopes of NOEMA (NOrthern Extended Millimetre Array) in France to find out more about how these early star factories managed to create so many stars. Yang and his colleagues measured light from two luminous galaxies in the early universe – one of them classified as a quasar, and both with high rates of star formation.
“We knew these galaxies were prodigious star factories, perhaps amongst the biggest the universe has ever seen. To be able to find out how they work, we measured their light at wavelengths around one millimetre hoping to collect new clues,” says Chentao Yang.
The measurements proved to be successful beyond the scientists’ expectations. In the light they recorded from both galaxies, they identified traces of many different kinds of molecules. From deep within these galaxies, light is emitted in many different wavelengths from the clouds of gas and dust where new stars are born.
“It’s an amazing explosion of colour, in shades that the human eye can’t see. But by combining our observations with our knowledge of physics and chemistry, we can understand what the colours mean, and see what differences there are between different galaxies,” explains Sergio Martín, astronomer at ESO and Joint ALMA Observatory, Chile, and member of the research team.
By analysing each galaxy’s spectrum – the individual colours of their light - the scientists were able to identify 13 molecules, several of which have never been seen before in such distant galaxies. Each molecule gives different clues about the temperature, pressure, and density in the space between the stars, and about how starlight, radiation and matter interact, providing key new information on the physical and chemical conditions in these galaxies.
“Interpreting the signals is a challenge. We are seeing part of the electromagnetic spectrum that is hard to observe in nearby galaxies. But thanks to the expansion of the universe, the light from distant galaxies like these is shifted to longer wavelengths that we can see with radio telescopes observing in the sub-millimetre”, says Chentao Yang.
The two galaxies studied by the team are so far away that their light takes almost 13 billion years to reach us.
“Looking at these galaxies is less like a night under the stars and more like seeing a city lit with neon lights”, says Susanne Aalto, Chalmers astronomer and team member.
Astronomers are used to taking pictures of our galaxy’s star factories, like the Orion Nebula and the Carina Nebula, she explains.
“In these two distant galaxies, we are instead seeing star factories that are bigger, brighter, full of dust, and different in many ways. The Orion and Carina nebulae are lit up thanks to ultraviolet light from hot, newborn stars. In these two distant galaxies, ultraviolet light can’t get past the layers of dust. Much of the illumination is instead thanks to cosmic rays – high energy particles that can be created by exploding stars or close to a supermassive black hole”, says Susanne Aalto.
“To help us understand our measurements, we ran computer simulations of a complex set of thousands of chemical reactions. Thanks to these calculations, we could begin to understand the dramatic chemistry going on in these galaxies, and in particular how the gas there is heated,” says astronomer Thomas Bisbas, astronomer at Zhejiang Lab in China.
While galaxies like these two are rare, the scientists have plans to study more of them, using both NOEMA and its even bigger sister telescope, ALMA (the Atacama Large Millimetre/Submillimetre Array) in Chile. Both telescopes are sensitive to light with wavelengths of around one millimetre.
“Our results show how NOEMA with its broadband receivers and powerful correlator computer has opened up new opportunities for studying extreme galaxies like these in the northern sky. From the southern hemisphere, ALMA’s planned Wideband Sensitivity Upgrades will offer even more exciting prospects. The most remarkable galaxies in the early universe are finally able to tell their stories through their molecules”, says Pierre Cox, astronomer at CNRS and Sorbonne Université, France.
More about the research results
Over a hundred different molecules have been detected in interstellar space. In this study, the astronomers identified molecules of carbon monoxide (CO), the cyano radical (CN), the ethynyl radical (CCH), hydrogen cyanide (HCN), the formyl cation (HCO+), hydrogen isocyanide (HNC), carbon monosulphide (CS), water (H2O), the hydronium ion (H3O+), nitric oxide (NO), diazenylium (N2H+), methylidyne radical (CH), and cyclopropenylidene (c-C3H2). Several of these (CH, CCH, c-C3H2, N2H+, and H3O+) have never been seen before at such large distances.
The two galaxies in the study have catalogue numbers APM 08279+5255 and NCv1.143. Previous studies have shown that they are so far away that their light has been traveling towards us for nearly 13 billion years, corresponding to redshifts of 3.911 and 3.565, respectively. Redshift means that the expansion of the universe stretches the light from distant galaxies to longer wavelengths, which can be observed with radio telescopes. Despite their distance, the galaxies shine brightly at radio wavelengths. Their signals are amplified thanks to clusters of other galaxies that lie along the light's path – an effect known as gravitational lensing. One of the galaxies, APM 08279+5255, is also a quasar, a galaxy whose centre glows brightly all the way from radio waves to X-rays, due to material swirling around a supermassive black hole. NCv1.143 may also contain a central black hole.
More about the research group and the paper
The research is presented in a paper, “SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys”, published in the journal Astronomy & Astrophysics. (Link to paper: https://www.aanda.org/10.1051/0004-6361/202347610)
The team is composed of Chentao Yang (Chalmers), Alain Omont (CNRS and Sorbonne Université, France), Sergio Martín (ESO and Joint ALMA Observatory, Chile), Thomas G. Bisbas (Zhejiang Laboratory, China), Pierre Cox (CNRS and Sorbonne Université, France), Alexandre Beelen (Aix Marseille Univ, France), Eduardo González-Alfonso (Universidad de Alcalá, Spain), Raphaël Gavazzi (Aix Marseille Univ), Susanne Aalto (Chalmers), Paola Andreani (ESO), Cecilia Ceccarelli (Univ. Grenoble Alpes, CNRS), Yu Gao (Xiamen University, China), Mark Gorski (Chalmers), Michel Guélin (IRAM, France), Hai Fu (University of Iowa, USA), Rob J. Ivison (ESO, Macquarie University, Dublin IAS, University of Edinburgh), Kirsten K. Knudsen (Chalmers), Matthew Lehnert (Centre de Recherche Astrophysique de Lyon—CRAL, France), Hugo Messias (ESO and Joint ALMA Observatory, Chile), Sebastien Muller (Chalmers), Roberto Neri (IRAM), Dominik Riechers (Universität zu Köln), Paul van der Werf (Leiden University, Netherlands) and Zhi-Yu Zhang (Nanjing University, China).
See also the press release from IRAM (English).
More about NOEMA
NOEMA, the Northern Extended Millimetre Array, is the most powerful millimetre observatory in the Northern Hemisphere, located on 2500 metres above sea level on the Plateau de Bure in the French Alps and run by IRAM. It consists of an array of 12 individual 15-metre antennas. During observations, the antennas function as a single telescope by using a technique called interferometry.
Contact
For more information, please contact:
Robert Cumming, astronomer and communicator, Onsala Space Observatory, Chalmers University of Technology, Sweden, robert.cumming@chalmers.se, +46 70 4933114
Chentao Yang, astronomer, Chalmers University of Technology, Sweden, chentao.yang@chalmers.se
Images
Contact us for high-resolution images.
Photographer: ESA/Hubble, NASA, L. Ho; Jmol (molecules); R. Cumming (montage)
Photographer: NASA, ESA & W. P. Maksym (CfA); Jmol (molecules); R. Cumming (montage)
Photographer: Chentao Yang et al.
Photographer: © IRAM/DiVertiCimes
- Communications Officer, Onsala Space Observatory, Space, Earth and Environment
