The scientists used the National Science Foundation's Very Long Baseline Array (VLBA), a continent - wide radio - telescope system, along with the 100 - meter radio telescope in Effelsberg, Germany, to make an extremely precise observation when the planet Jupiter passed nearly in front
of a bright quasar on September 8, 2002.
Not exact matches
Quasars are
bright disks
of gas and dust swirling around supermassive black holes.
The question is, Which channel created the bulk
of the
bright ancient
quasars that astronomers see?
And starting with seeds in this range alleviates the timing problem for the production
of the supermassive black holes that power the
brightest, most distant
quasars.
The two black holes live roughly 3.7 billion light - years away in a
quasar, the ferociously
bright core
of a galaxy lit up by...
Quasars are
bright cores
of distant active galaxies.
And when
quasars [extremely
bright, compact objects at the centers
of some galaxies] were discovered in the early 1960s, it was obvious that the source
of power had to be gravitational because even nuclear power, which powers the stars, is too inefficient.
The only way to make the
quasars so
bright, astronomers believe, is for supermassive black holes to devour gas at the hearts
of large galaxies.
But the realization that
quasars were really out at the edge
of the observable universe, and thus must be far
brighter than the
brightest galaxy, posed a riddle that nobody has yet been able to answer with certainty: What are they?
It is the first time that a survey
of quasars shows such
bright halos around all
of the observed
quasars.
When the
bright cosmic beacons known as
quasars try to devour too much gas, they spew some
of it deep into space in fierce jets.
Researchers were able to study the
quasar (seen above) in detail, thanks to the magnifying effect
of a gravitational lens — a massive galaxy cluster in front
of it — that caused it to appear
brighter than it would have otherwise.
The images revealed a
bright quasar, the energetic signature
of a black hole, residing far from the galactic core.
Quasars are incredibly
bright powerhouses
of radiation that are believed to be fueled by gas falling into a massive black hole at the core
of a galaxy.
The ideal background «lights» for such a study are
quasars, which are very distant
bright cores
of active galaxies powered by black holes.
Previous research suggested these giants release extraordinarily large amounts
of light when they rip apart stars and devour matter, and likely are the driving force behind
quasars, which are among the
brightest objects in the universe.
The first clue that supermassive black holes exist was the discovery several decades ago
of quasars — extremely
bright objects in the centres
of distant galaxies.
Shining with the equivalent
of 420 trillion suns, the new
quasar is seven times
brighter than the most distant
quasar known (which is 13 billion years away).
Quasars can be hundreds
of times as
bright as their surrounding galaxy, yet they are smaller than our Solar System.
But recently, a survey has found several
quasars —
bright cores
of galaxies, powered by matter falling into a supermassive black hole — that existed less than a billion years after the big bang.
Added Bram Venemans
of the Max Planck Institute for Astronomy in Germany: «
Quasars are among the
brightest and most - distant known celestial objects and are crucial to understanding the early universe.»
Quasars are tremendously
bright objects composed
of enormous black holes accreting matter at the centers
of massive galaxies.
Quasars are among the
brightest and most - distant known celestial objects and are crucial to understanding the early Universe, added Bram Venemans
of the Max Planck Institute for Astronomy in Germany.
Bañados was looking in particular for
quasars — some
of the
brightest objects in the universe, that consist
of a supermassive black hole surrounded by swirling, accreting disks
of matter.
Between 20 and 100
quasars as
bright and as distant as the
quasar discovered by Bañados and his team are predicted to exist over the whole sky, so this is a major discovery that will provide fundamental information
of the young universe, when it was only 5 percent its current age.
Astronomers had been able to spot the signature
of specific molecules in the early universe before, but those observations were mostly confined to extremely
bright objects such as
quasars.
«The
brightest quasars, probably hosting the most massive black holes, don't necessarily have to live in the densest regions
of the universe,» she said.
Unimaginably powerful sources
of radio emissions,
brighter than entire galaxies,
quasars were initially viewed as mysterious objects found billions
of light - years from us but unknown in our own galactic neighborhood.
«We had expected we would see faint emissions right on top
of the
quasar, and instead we saw strong
bright carbon emission from the galaxies at large separations from their background
quasars,» said J. Xavier Prochaska, professor
of astronomy and astrophysics at UC Santa Cruz and coauthor
of the paper.
«However, the
quasars are not
bright enough now to account for what we're seeing; this is a record
of something that happened in the past,» Keel said.
Quasars, discovered in 1963, are extremely distant massive black holes (MBHs) whose gravity pulls in immense amounts of nearby matter.24 The potential energy of all that infalling matter is converted to bright radiation, making quasars the most luminous stable objects in the un
Quasars, discovered in 1963, are extremely distant massive black holes (MBHs) whose gravity pulls in immense amounts
of nearby matter.24 The potential energy
of all that infalling matter is converted to
bright radiation, making
quasars the most luminous stable objects in the un
quasars the most luminous stable objects in the universe.
«Thirty - seven
of the
brightest galaxies were detected, including a
quasar, but thousands
of galaxies were probably in the string, according to astronomer Dr. Paul Francis who heads the team.
However,
quasars are so rare and the nearest is so remote that the
brightest of them, 3C273, about 2 billion lightyears away in the constellation Virgo, is only
of magnitude 13.7, and none
of them is in Messier's or even in the NGC or IC catalog.
So, instead
of relying on this method, Melis» team used radio measurements to perform the work, which opened up a more reliable distance beacon:
quasars, amazingly
bright galactic cores powered by supermassive black holes.
Astronomers have discovered a new type
of quasar — an incredibly
bright galactic core powered by a supermassive black hole — that current theory fails to predict.
The plane to the far right shows the background galaxy and overlaid in the center
of the galaxy is a
bright white light representing a
quasar.
Although
quasars can be very
bright, they are rare and are comparatively small, only a fraction
of a light year across, whereas galaxies are quite common and provide a 100 million-fold increase in area to probe DLAs.
Astronomers also looked at how the light coming out certain
of bright, distant galaxies, called
quasars, filtered through these cobwebby strands.
The first stars lit up a few - hundred - million - years - long «Dark Age» with spectacular intensity, leading to the rapid creation
of heavy elements and black holes that coalesced to form
bright quasars (more).
Indeed, GRBs appear to emit produce even more energy than supernovae or even
quasars (which are energetically
bright accretion disks and bi-polar jets around supermassive black holes that are most commonly found in the active nuclei
of some distant galaxies and possibly even in the pre-galaxy period after the Big Bang).
The remote
quasars are so
bright that they drown out light emitted by stars in their proto - galactic clump
of stars (more illustrations).
Analysis
of data collected by the Hubble and Chandra space telescopes and the Sloan Digital Sky Survey showed a
bright quasar located far from its galaxy's core.
This deep image shows the nebula (cyan) extending across 2 million light - years that was discovered around the
bright quasar UM287 (at the center
of the image).
New radio images
of galaxies with
bright quasar cores show that, though the galaxies appear normal in visible - light images, their gas has been disrupted by encounters with other galaxies.
Subsequently, however, an even more distant
quasar with a tentative redshift
of z = 6.40 was announced on January 9, 2003, near the SDSS detection limit
of a redshift
of z ~ 6.5 for
bright quasars, and other teams
of astronomers detected even more distant, fast - star - forming irregular proto - galaxies, including: gravitationally - lensed HCM 6A behind galaxy cluster Abell 370 with a redshift
of z ~ 6.56, which appears to be converting about 40 Solar - masses into stars annually; (PhysicsWeb; IFA press release; Hu et al, 2002, in pdf; and erratum); and the possible «superwind - galaxy» LAE J1044 - 0130 (Subaru press release; and Ajiki et al, 2002, in pdf).
«However, the
quasars are not
bright enough now to account for what we're seeing; this is a record
of something that happened in the past,» Bill Keel
of the University
of Alabama, Tuscaloosa, who initiated the Hubble survey, said in a statement.
The four
quasars — extremely
bright masses
of light and energy that exist only in the farthest reaches
of the known universe — were found huddled together in a nebula 10 billion light - years away, the first time four
quasars have ever been spotted so close together, according to the atronomers» findings published Friday in the journal Science.
The galaxy hosts a
bright quasar that may have illuminated the ghostly structure by hitting it with a beam
of light from hot gas around a central black hole.
The halos around
quasars — the
brightest and the most active objects in the universe, they are galaxies formed less than 2 billion years after the Big Bang; they have supermassive black holes in their centers and consume stars, gas, interstellar dust and other material at a very fast rate — are made
of gas known as the intergalactic medium and extend for up to 300,000 light - years from the centers
of the
quasars.
The observation
of these
quasars, selected from among the
brightest observable by MUSE, threw up another surprising find.