Ten times more hyper luminous galaxies observed than stars can produce

A team of astronomers led by SRON has observed ten times more hyper luminous galaxies in the infrared than stars can produce according to the models. If the theory is correct, it means that stars alone cannot account for the brightness of the most luminous infrared galaxies. Publication in a special issue of Astronomy & Astrophysics. On ArXiv on November 18th.

After the Universe emerged from the Big Bang 13.8 billion years ago, galaxies filled with stars began to form relatively quickly around three billion years later. There was plenty of gas to go around, so a small portion of these early galaxies were able to grow into massive, hyper luminous galaxies, with a brightness of ten trillion suns. As the gas reserves grew empty with time, fewer galaxies could grow at a fast pace.

When astronomers observed the Universe with the infrared space telescope Herschel, they found that this theory largely checks out. However, in terms of absolute numbers it looked like there are over an order of magnitude too many hyper luminous infrared galaxies, both in the early Universe and more recent epochs. Unfortunately Herschel's spatial resolution couldn't resolve all individual galaxies, so they couldn't say for sure.

An international team of astronomers, led by Lingyu Wang from SRON and RUG, has now used the LOFAR telescope—with higher spatial resolution—to distinguish galaxies individually. They found that indeed there are over an order of magnitude more hyper luminous galaxies than the theory predicts. With an uncertainty of a factor two they can say for sure that we need to look for a different theory.

Image 1: The observed spectrum and the fitting spectrum of an example hyper luminous galaxy. Along the bottom of the plot, we also show the images of this galaxy in different wavelengths. From left to right: HSC i-band (optical), DXS K-band (near-infrared), IRAC 4.5 μm (mid-infrared), MIPS 24 μm (far-infrared), Herschel SPIRE 250 μm (far-infrared), and LOFAR 2 m (radio). It shows that hyper luminous infrared galaxies are usually very faint or even undetected in optical data and emit most of their energy in the infrared.

'We are now studying what physical mechanisms can power such extreme galaxies,' says Wang. 'Are they powered by star formation or by supermassive black hole accretion? If powered by star formation, hyper luminous infrared galaxies would be forming stars at a few thousands solar masses per year. Theoretical models cannot produce that many galaxies forming stars at such extreme rates. So, an alternative scenario is that they are predominantly powered by accretion activity around the central black hole. We need more follow-up observations to study the true nature of these extreme objects.'

The team will perform this follow-up study using the Keck observatory. It will give them more accurate data on galaxies' redshift and therefore their distance. Keck harbors an optical telescope, providing spectra. Astronomers deduce the redshift from spectra by looking at how many wavelengths the characteristic fingerprints have shifted.