ESA Science & Technology - Herschel discovers mature galaxies in the young Universe

Lensed image of galaxy S0901. Credit: NASA/STScI; S. Allam and team; and the Master Lens Database (masterlens.org), L. A. Moustakas, K. Stewart, et al. (2014)

When galaxies form, they accumulate mass by gravitationally attracting vast, external gas clouds. As the gas clouds enter the galaxy, they fall into haphazard orbits. These disordered paths cause turbulence in the host galaxies, which can drive star formation.

To investigate the internal conditions of forming galaxies James Rhoads and Sangeeta Malhotra, both from Arizona State University, and colleagues targeted two young galaxies, known as S0901 and the Clone. The light from both galaxies has taken 10 billion years to reach us across space. Thus, we are seeing them when they were comparatively young.

"The purpose of this project is to study the physical conditions of gas in those galaxies. We wanted to know: are they similar to the galaxies around us or is there some difference in their physical conditions," says Rhoads.

The two galaxies they choose to study are average galaxies for that time in cosmic history. This means that they are about 10-20 per cent the size of our Milky Way, which is considered an average galaxy in the present-day Universe.

Studying galaxies so far away is usually hampered because they appear too dim to study effectively but in this case, the researchers were helped by a cosmic magnifier known as a gravitational lens. The two galaxies both sit behind intervening groups of galaxies, whose gravity warps space. As described by Albert Einstein's General Theory of Relativity, this warping acts like a lens. Although it distorts the images of the young galaxies, it helps by magnifying their light, thus bringing them within reach of Herschel's HIFI instrument.

Herschel spectrum of the galaxy S0901. Credit: ESA/Herschel/HIFI. Acknowledgments: James Rhoads and Sangeeta Malhotra, Arizona State University, USA

The researchers used HIFI to investigate the infrared light of ionized carbon, which is emitted at a wavelength of 158 micrometres (a frequency of 1900 GHz). This spectral line is produced in the clouds that surround star-forming regions. HIFI showed the line was broadened into a double peak, and this allowed the motion of the gas to be fitted with a model.

Firstly, the team fitted the overall rotation of the galaxy, and then the turbulence in the gas clouds. To their surprise they found that galaxy S0901 was extremely well behaved. Instead of turbulence, it was found to be in orderly rotation, much more akin to the majestic galaxies of today.

"Usually, when astronomers examine galaxies at this early era, they find that turbulence plays a much greater role than it does in modern galaxies. But S0901 is a clear exception to that pattern, and the Clone could be another," says Rhoads.

The Clone, the second galaxy in their study, could also be fitted by an orderly rotation. However, because it was somewhat dimmer, the quality of the data was not so good. This meant that the data could also be fitted with a highly turbulent model, as conventional wisdom would expect.

Herschel spectrum of the Clone. Credit: ESA/Herschel/HIFI. Acknowledgments: James Rhoads and Sangeeta Malhotra, Arizona State University, USA

"Galaxies 10 billion years ago were making stars more actively than they do now," says Malhotra, "They usually also show more turbulence, likely because they are accumulating gas faster than a modern galaxy does. But here we have cases of early galaxies that combine the 'calm' rotation of a modern one with the active star formation of their early peers. This suggests first that these galaxies have finished accumulating their gas, at least for now. But it also seems that turbulence is not actually required to trigger that early, active star formation."

Malhotra acknowledges the preliminary nature of their study. "This is not the last word on this. We need a bigger sample to be sure of our conclusions," she says.

But that bigger sample will not be investigated by Herschel. As predicted, the liquid helium coolant needed to keep HIFI and Herschel's other instruments working ran out in April 2013. Instead the researchers hope to continue the work pioneered by Herschel using the Atacama Large Millimeter/submillimeter Array (ALMA), a ground-based array of 66 radio dishes in Chile.

"It is mind-boggling that with Herschel/HIFI – admittedly with the help of gravitational lensing – it has been possible to study the internal gas kinematics in galaxies when the Universe was only a few billion years old, and what we can learn about them this way. This pioneering work by Herschel is bound to be continued," says Göran Pilbratt, Herschel Project Scientist at ESA.

Background Information

The study reported here is based on observations performed with the Heterodyne Instrument for the Far-Infrared (HIFI) on board ESA's Herschel Space Observatory of SDSS090122.37+181432.3, referred to as S0901, and SDSS J120602.09+514229.5, known as the Clone. The results are published in "Herschel Extreme Lensing Line Observations: Dynamics of two strongly lensed star forming galaxies near redshift z = 2", by J. Rhoads et al., to appear in the 2014 May 20 issue of The Astrophysical Journal, volume 787, issue 1.

Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

The HIFI instrument is a very high-resolution heterodyne spectrometer and operates in seven bands covering the wavelength range between 157 and 625 µm. HIFI has been designed and built by a consortium of institutes and university departments across Europe, Canada, and the United States under the leadership of SRON Netherlands Institute for Space Research, the Netherlands, with major contributions from Germany, France, and the USA. HIFI Consortium members are: CSA, U. Waterloo (Canada); CESR, LAB, LERMA, IRAM (France); KOSMA, MPIfR, MPS (Germany); NUI Maynooth (Ireland); ASI, IFSI-INAF, Osservatorio Astrofisico di Arcetri-INAF (Italy); SRON, TUD (Netherlands); CAMK, CBK (Poland); Observatorio Astronómico Nacional (IGN), Centro de Astrobiología (CSIC-INTA) (Spain); Chalmers University of Technology - MC2, RSS & GARD, Onsala Space Observatory, Swedish National Space Board, Stockholm University - Stockholm Observatory (Sweden); ETH Zurich, FHNW (Switzerland); Caltech, JPL, NHSC (USA).

Herschel was launched on 14 May 2009 and completed science observations on 29 April 2013.

Contacts

James Rhoads
School of Earth and Space Exploration
Arizona State University
Tempe, AZ 85287, USA
Email: James.Rhoadsasu.edu
Phone: +1-480-727-7133

Sangeeta Malhotra
School of Earth and Space Exploration
Arizona State University
Tempe, AZ 85287, USA
Email: Sangeeta.Malhotraasu.edu
Phone: +1-480-965-2552

Göran Pilbratt
Herschel Project Scientist
Scientific Support Office
Science and Robotic Exploration Directorate
ESA, The Netherlands
Email: gpilbrattrssd.esa.int
Phone: +31-71-565-3621