Powerful radio jets from
the supermassive black hole at the center of the galaxy are creating giant radio bubbles (blue) in the ionized gas surrounding the galaxy.
A century later, that insight underpins cutting - edge physics: searching for gravitational waves, probing the extreme gravity near
the supermassive black hole at the center of our galaxy, tracing the origin of the universe.
Resembling spotlights at a Hollywood movie premier, such beams are probably generated as matter plunges into
a supermassive black hole at the center of the galaxy.
New observations from ESO's Very Large Telescope show for the first time a gas cloud being ripped apart by
the supermassive black hole at the center of the galaxy.
The radio waves in question come from quasars, which are
supermassive black holes at the center of galaxies billions of light years away from Earth.
Supermassive black holes at the centers of galaxies formed in lockstep with the stellar structures of the galaxies.
On the evening of July 3, 2014, both of the mighty 10 - meter Keck Observatory telescopes were steered by Dr. Andrea Ghez and her team of observers from the UCLA Galactic Center Group to study
the supermassive black hole at the center of our galaxy.
See images of new observations from ESO's Very Large Telescope showing a gas cloud ripped apart by
the supermassive black hole at the center of our galaxy, the Milky Way.
An international research team led by Takuma Izumi, a second - year master's student of science at the University of Tokyo, and Kotaro Kohno, a professor at the University of Tokyo, successfully captured a detailed image of high - density molecular gas around an active
supermassive black hole at the center of a galaxy called NGC 1097 at the highest sensitivity ever achieved.
Figure 1 Composite image showing how powerful radio jets from
the supermassive black hole at the center of a galaxy in the Phoenix Cluster inflated huge «bubbles» in the hot, ionized gas surrounding the galaxy (the cavities inside the blue region imaged by NASA's Chandra X-ray observatory).
Maunakea, Hawaii — Stars forming in galaxies appear to be influenced by
the supermassive black hole at the center of the galaxy, but the mechanism of how that happens has not been clear to astronomers until now.
Artist's conception of the pair of
supermassive black holes at the center of the galaxy 0402 +379, 750 million light - years from Earth.
When
supermassive black holes at the center of galaxies accrete matter (usually gas), they give rise to a highly energetic phenomena named Active Galactic Nuclei (AGN).
The «virtual telescope» is first getting up close and personal with Sagittarius A *,
the supermassive black hole at the center of our galaxy.
Then, the team behind the new paper compared those ages with the size of
the supermassive black hole at the center of the galaxies those stars live in, which other scientists had previously calculated.
Quasars are among the most luminous objects in the universe, and generally are believed to be powered by material being drawn into
a supermassive black hole at the center of a galaxy, releasing large amounts of energy.
Hubble also probed the cores of collisions, showing that interactions fuel
supermassive black holes at the centers of galaxies.
The supermassive black hole at the center of our galaxy is hidden behind dense clouds of dust and gas.
The picture, pinned above his desk, shows a bright orange and yellow blob — the glow of cosmic gas as it gets devoured by
the supermassive black hole at the center of the galaxy.
Not exact matches
Yes, we have the telescopes to measure the positions
of stars orbiting the
supermassive black hole located
at the
center of our
galaxy.
A
supermassive black hole, like the one illustrated above, lurks
at the
center of our
galaxy, deceptively quiet.
Powerful radiation from
supermassive black holes at the
center of most large
galaxies creates winds that can blow gas out
of the
galaxies, halting star formation.
As matter falls toward the
supermassive black hole at the
galaxy's
center, some
of it is accelerated outward
at nearly the speed
of light along jets pointed in opposite directions.
Over the past several decades, though, astronomers have realized that
black holes are not so unusual after all:
Supermassive ones, millions or billions
of times as hefty as the sun, seem to reside
at the
center of most, if not all,
galaxies.
The objects causing these low - frequency ripples — such as orbiting
supermassive black holes at the
centers of distant
galaxies — would be different from the higher frequency ripples, emitted by collisions
of much smaller
black holes, that have so far been detected on Earth.
These ultra-compact dwarfs are around 0.1 percent the size
of the Milky Way, yet they host
supermassive black holes that are bigger than the
black hole at the
center of our own
galaxy,» marvels Ahn.
Supermassive black holes have a mass
of more than 1 million suns, and are thought to be
at the
center of all big
galaxies.
After charting stars in the heart
of our
galaxy traveling
at speeds up to 50 times faster than Earth circles the sun, scientists are convinced that a
supermassive black hole is pulling the strings, as only the relentless grip
of a
supermassive black hole could keep these frenzied stars locked into orbit within the galactic
center.
Supermassive black holes, which can be hundreds
of thousands to billions
of times more massive than the sun, may be found
at the
center of most
galaxies.
Scientists also believe there could be a
supermassive black hole at the
center of nearly every
galaxy, including our own.
The vast majority
of supermassive black holes lurk quietly
at the
centers of their
galaxies, not betraying their presence except through the pull
of gravity.
A small fraction
of supermassive black holes — the ginormous ones that lurk
at the
centers of galaxies — fire off light - speed jets
of particles as they snack.
Astronomers have seen them shooting out
of young stars just being formed, X-ray binary stars and even the
supermassive black holes at the
centers of large
galaxies.
To measure the mass and growth rate
of these
galaxies» active nuclei — the
supermassive black holes at the
galaxies»
centers — the researchers used data from 12 different ground - based telescopes spread across the globe to complement the data from the Swift satellite.
Researchers expect to directly measure this phenomenon beginning in the spring as S0 - 2 makes its closest approach to the
supermassive black hole at the
center of our Milky Way
galaxy.
Quasars are caused by the close encounter
of two
supermassive black holes, each with billions
of solar masses and crammed into tight quarters
at the
center of a
galaxy.
«The electrons that make up the cloud initially bounce off the
supermassive black hole at the
center of one
of the
galaxies and accelerate as a result.
At the
center of our
galaxy, in the immediate vicinity
of its
supermassive black hole, is a region wracked by powerful tidal forces and bathed in intense ultraviolet light and X-ray radiation.
The joint research team led by graduate student and JSPS fellow Takuma Izumi
at the Graduate School
of Science
at the University
of Tokyo revealed for the first time — with observational data collected by ALMA (Atacama Large Millimeter / submillimeter Array), in Chile, and other telescopes — that dense molecular gas disks occupying regions as large as a few light years
at the
centers of galaxies are supplying gas directly to the
supermassive black holes.
Supermassive black holes more than a million times the mass
of our sun exist
at the
centers of many
galaxies, but how they came to be is unclear.
«We think most large
galaxies have a
supermassive black hole at their
center, but they are too far away for us to study how matter flows near it,» said Q. Daniel Wang
of the University
of Massachusetts in Amherst, who led
of a study published Thursday in the journal Science.
Supermassive black holes lurk at the centers of galaxies, and when those galaxies collide, eventually their supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually me
Supermassive black holes lurk
at the
centers of galaxies, and when those
galaxies collide, eventually their
supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually me
supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually merge as well.
Their VLBA observations showed that the
supermassive black holes of nearly all these
galaxies were
at the
centers of the
galaxies.
The gas outflow driven by a
supermassive black hole at the galactic
center recently has become the focus
of attention as it possibly is playing a key role in the co-evolution
of galaxies and
black holes.
VLBA images detect orbital motion
of two
supermassive black holes as they circle each other
at the
center of a distant
galaxy.
The discovery was made as part
of a program to detect
supermassive black holes, millions or billions
of times more massive than the Sun, that are not
at the
centers of galaxies.
Supermassive black holes reside
at the
centers of most
galaxies.
Quasars are very luminous objects powered by accretion
of gas into
supermassive black holes at the
centers of distant
galaxies.
The second will study the formation, growth and ultimate sizes
of the
supermassive black holes found
at the
centers of galaxies.
Astronomers have previously suggested that these so - called primordial
black holes could account for all or some
of the universe's mysterious dark matter and that they might have seeded the formation
of supermassive black holes that exist
at the
centers of galaxies.