He and his colleagues found that gas - rich galaxies — common in the early universe — may be the key to the formation of
early supermassive black holes.
The other possibility is that
early supermassive black holes simply broke the Eddington limit.
As such, researchers want to look at as many
early supermassive black holes as possible to learn more about their growth and their effects on the rest of the cosmos.
OBESE black holes, not stars, may have lit up the first galaxies — and could have grown into
the earliest supermassive black holes.
The earliest supermassive black holes were first sighted in 2001 through a telescope at New Mexico's Apache Point Observatory as part of the Sloan Digital Sky Survey.
To further unveil the nature of this remarkable quasar, and to shed light on the physical processes that led to the formation of
the earliest supermassive black holes, the research team will carry out further investigations on this quasar with more international telescopes, including the Hubble Space Telescope and the Chandra X-ray Telescope.
The earliest supermassive black holes may have been big to start with.
The observations, presented in a paper led by Yali Shao (Peking University and the National Radio Astronomy Observatory), have provided intriguing insight about
early supermassive black hole growth.
Not exact matches
The existence of
supermassive black holes in the
early universe has never made much sense to astronomers.
And putting together a census of binary
supermassive black holes from the
early universe, he adds, might help researchers understand what role (if any) these dark duos had in shaping galaxies during the billion or so years following the Big Bang.
Computational analysis of Sloan's prodigious data set has uncovered evidence of some of the
earliest known astronomical objects, determined that most large galaxies harbor
supermassive black holes, and even mapped out the three - dimensional structure of the local universe.
The findings have scientists puzzling over how
early black holes grew into the
supermassive beasts they are today without a steady diet of gas, dust, stars, and other fodder.
Though relatively rare, enough galaxies of this size exist in the
early universe to explain the
supermassive black holes observed so far.
This process is likely stopped
early on by powerful gas outflows from supernova explosions, stellar winds and possibly even from the central
supermassive black hole.
Evidence for
supermassive black holes — weighing millions or billions of suns — has been found in the
early universe, but no one knows how they grew so big so fast.
«Knowing more about the
black holes powering quasars will allow us to know more about how galaxies develop,» said Marta Volonteri, the research director at the Observatory of Paris and the principal investigator of the BLACK project, which investigates how supermassive black holes influenced their host galaxies, especially as quasars, in the early univ
black holes powering quasars will allow us to know more about how galaxies develop,» said Marta Volonteri, the research director at the Observatory of Paris and the principal investigator of the
BLACK project, which investigates how supermassive black holes influenced their host galaxies, especially as quasars, in the early univ
BLACK project, which investigates how
supermassive black holes influenced their host galaxies, especially as quasars, in the early univ
black holes influenced their host galaxies, especially as quasars, in the
early universe.
«This ultraluminous quasar with its
supermassive black hole provides a unique laboratory to the study of the mass assembly and galaxy formation around the most massive
black holes in the
early universe.»
Supermassive black holes in the cores of galaxies are thought to fatten slowly over eons, so finding such a heavyweight so
early in the history of the universe is «really pushing it,» he says.
And
earlier this year, astronomers showed that the
early, distant universe is missing the glow of x-ray light that would be expected from a multitude of small
black holes — another sign favoring the sudden birth of big seeds that go on to be
supermassive black holes.
TOO BIG, TOO SOON
Supermassive black holes that are actively feeding on gas and dust, like the one shown in this artist's rendition, have been spotted in the
early universe — before they should have had time to grow.
FIRST BURST A
supermassive black hole (illustrated) in the
early universe suggests some
black holes got a head start on the galaxies they inhabit.
Astronomers have measured Eddington ratios for only about 20
supermassive black holes in the
early universe.
It was strange enough to find
supermassive black holes with gluttonous appetites in the
early universe, but these picky eaters are even harder to explain.
Such «supercritical accretion» is thought to be a possible mechanism in the formation of
supermassive black holes at galactic centers in very short time periods (which are observed very
early in cosmic time).
«Infant stars found surprisingly near galaxy's
supermassive black hole:
Earliest phase of star formation ever observed in highly hostile environment.»
Supermassive black holes take a long time to build, so we expect to see only a few in the
early universe.
ALMA discovers remarkably
early signs of low - mass star formation near the
supermassive black hole at the center the Milky Way.
That takes time, yet somehow the
early universe contained
supermassive black holes, hundreds of thousands of times larger than our sun.
u «Astronomers are puzzled about how the oldest
supermassive black holes could have grown so big so
early in cosmic history.»
This meeting brings together scientists from across Europe, whose aim is to detect the gravitational wave signature from interacting
supermassive black holes in distant, merging galaxies in the
early universe.
This could potentially explain how
supermassive black holes attained masses of a billion times the sun in the
early days of the universe, when it was just about one billion years old.
We now know that galaxies began dying fairly
early in the history of the universe, and that central
supermassive black holes and galactic collisions play key roles in galactic evolution.
One explanation for the existence of
supermassive black holes in the
early universe postulates that the first
black holes were «seeds» that grew into much larger
black holes by gravitationally attracting and then swallowing matter.
The
supermassive black holes that lie in the center of most galaxies may have far more voracious appetites than experts previously believed, according to a new study that has uncovered evidence that these behemoths shred stars 100 times more often than
earlier research had suggested.
But, in the
early universe, their study shows that the 3C 298 galaxy is 100 times less massive than it should be given its behemoth
supermassive black hole mass.
The
supermassive black hole formed during the
earliest moments of the universe, which has researchers puzzled over how it got to be so big.
How did the first
supermassive black holes grow alongside their host galaxies in the
early universe?
«There's a challenge in how do you explain the presence of
supermassive black holes... so
early in the universe?
Or could this provide us with insight into how all
supermassive black holes grew in the
early universe?
The mechanisms behind
black hole accretion are poorly understood, but the researchers suggest that this example may just have been an «
early bloomer» that had an extremely active youth, only to settle down as a «regular»
supermassive black hole in a large elliptical galaxy.
An artist's impression of a growing
supermassive black hole located in the
early Universe is seen in this NASA handout illustration released on June 15, 2011.
Supermassive black holes lurking in the hearts of countless galaxies are growing faster than astronomers suspected based on
earlier studies.
Quasars were such powerful generators of radiation in the
early universe because the
supermassive black holes in their cores had access to a huge quantity of material.
Using data from three of NASA's Great Observatories (the Hubble Space Telescope, Chandra X-ray Observatory, and Spitzer Space Telescope), scientists have found the best evidence to date that
supermassive black holes in the
early universe were produced by the direct collapse of a gas cloud.
Supermassive black holes can be relatively tranquil or they can flare up and drive incredibly powerful jets of subatomic particles deep into intergalactic space; quasars seen in the very
early Universe are an extreme example.
Dan P. Marrone is interested in galaxy clusters, galaxy formation in the
early universe, and the physics of the
supermassive black hole in our galaxy, Sagittarius A *.