“The gates of hell, the end of space and time,” was how black holes were described at the press conference in Brussels where the first ever photograph of one in galaxy M87 was revealed in April 2019. A new image has just be released by the European Southern Observatory (ESO) of a black hole and its halo at the dawn of the cosmos at redshift 6.2, meaning they are being seen as they were 12.8 billion years ago.
The gas halos newly observed with the MUSE instrument on ESO’s Very Large Telescope shown above is superimposed to an older image of a galaxy merger obtained with the ALMA array. The large-scale halo of hydrogen gas is shown in blue, while the ALMA data is shown in orange. The halo is bound to the galaxy, which contains a quasar at its center.
The faint, glowing hydrogen gas in the halo provides the perfect food source for the supermassive black hole at the center of the quasar. While quasars are bright, the gas reservoirs around them are much harder to observe. But MUSE could detect the faint glow of the hydrogen gas in the halos, allowing astronomers to finally reveal the food stashes that power supermassive black holes in the early Universe.
Primordial Galaxies –The Puzzle
“We are now able to demonstrate, for the first time, that primordial galaxies do have enough food in their environments to sustain both the growth of supermassive black holes and vigorous star formation,” says Emanuele Paolo Farina, of the Max Planck Institute for Astronomy in Heidelberg, Germany, who led the research published today in The Astrophysical Journal. “This adds a fundamental piece to the puzzle that astronomers are building to picture how cosmic structures formed more than 12 billion years ago.”
“The presence of these early monsters, with masses several billion times the mass of our Sun, is a big mystery,” says Farina, who is also affiliated with the Max Planck Institute for Astrophysics. It means that the first black holes, which might have formed from the collapse of the first stars, must have grown very fast. But, until now, astronomers had not spotted ‘black hole food’—gas and dust—in large enough quantities to explain this rapid growth.
To complicate matters further, previous observations with ALMA, the Atacama Large Millimeter/submillimeter Array, revealed a lot of dust and gas in these early galaxies that fueled rapid star formation. These ALMA observations suggested that there could be little left over to feed a black hole.
ESO’s Very Large Telescope in the Chilean Atacama Desert
To solve this mystery, Farina and his colleagues used the MUSE instrument on ESO’s Very Large Telescope in the Chilean Atacama Desert to study quasars—extremely bright objects powered by supermassive black holes which lie at the center of massive galaxies.
The study surveyed 31 quasars that are seen as they were more than 12.5 billion years ago, at a time when the Universe was still an infant, only about 870 million years old. This is one of the largest samples of quasars from this early on in the history of the Universe to be surveyed.
The astronomers found that 12 quasars were surrounded by enormous gas reservoirs: halos of cool, dense hydrogen gas extending 100 000 light years from the central black holes and with billions of times the mass of the Sun. The team, from Germany, the US, Italy and Chile, also found that these gas halos were tightly bound to the galaxies, providing the perfect food source to sustain both the growth of supermassive black holes and vigorous star formation.
The research was possible thanks to the superb sensitivity of MUSE, the Multi Unit Spectroscopic Explorer, on ESO’s VLT, which Farina says was “a game changer” in the study of quasars. “In a matter of a few hours per target, we were able to delve into the surroundings of the most massive and voracious black holes present in the young Universe,” he adds. While quasars are bright, the gas reservoirs around them are much harder to observe. But MUSE could detect the faint glow of the hydrogen gas in the halos, allowing astronomers to finally reveal the food stashes that power supermassive black holes in the early Universe.
In the future, ESO’s Extremely Large Telescope will help scientists reveal even more details about galaxies and supermassive black holes in the first couple of billion years after the Big Bang. “With the power of the ELT, we will be able to delve even deeper into the early Universe to find many more such gas nebulae,” Farina concludes.
This research is presented in a paper to appear in The Astrophysical Journal: The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars, arxiv.org/abs/1911.08498 arxiv.org/abs/1911.08498
The Daily Galaxy, Max Goldberg via ESO
Image credit: ESO/Farina et al.; ALMA (ESO/NAOJ/NRAO), Decarli et al.