Astronomers have found a relatively tiny galaxy whose black - hole - powered central engine is pouring out energy at a rate equal to that of
much larger galaxies, and they're wondering how it manages to do so.
He and his colleagues argue that these uniquely dense galaxies were once
much larger galaxies, but have been tidally stretched and disrupted by neighbouring galaxies in their crowded environment.
DWARF galaxies orbiting
the much larger galaxy Centaurus A appear to be moving along the same plane as one another.
In addition, this object is speeding away from the core of
a much larger galaxy, leaving a wake of ionized gas behind it.
The black hole surrounded by the small galactic remnant is currently speeding away from the core of
the much larger galaxy, and will continue to lose more mass as it does so.
Not exact matches
With all our knowledge, big brains, university degrees and amazing (to us) technology, consider than we dwell on a damp little planet, in an ordinary solar system, in the boonies of a very ordinary spiral
galaxy which is composed of billions of stars, millions of which are
much,
much larger than our sun.
Astronomers studying a nearby dwarf
galaxy have detected
large organic molecules, suggesting that the basic chemical building blocks of life can form in places
much more primitive than our own
galaxy.
The only way these outer regions could remain intact was if they were bound together by the gravitational embrace of a
much larger halo of invisible material, five to 10 times as massive as the visible
galaxy.
Tipping the scales at less than about a million suns in mass, middleweight black holes may hold clues to how their
much larger siblings, and
galaxies, first formed
And that made it possible for the researchers via Hubble and VLT to study in detail the distribution of stars in the
galaxy as well as the patterns of stellar rotation, says Sune Toft: «Thanks to the natural lens we were able to to gaze into the core of this
galaxy, which would otherwise have appeared not
much larger than a star to our telescopes.
However, Lauer says that the net velocity of the clusters indicates that the clumping of
galaxies is occurring on a
much larger scale than that found by Geller and Huchra.
«The process of generating galactic winds is something that requires exquisite resolution over a
large volume to understand —
much better resolution than other cosmological simulations that model populations of
galaxies,» Robertson said.
From her perspective, though, the real interest lies in a
much larger but sparser spherical cloud of stars, known as the spheroid, surrounding such
galaxies.
Herschel spotted two
large galaxies — 11 billion light - years away — in close proximity to one another, both of them making new stars at a
much higher rate than most
galaxies from that cosmic period.
Now, in a
much larger study and using a different technique, astronomer Michele Cappellari of the University of Oxford in the United Kingdom and his colleagues have confirmed and strengthened the conclusion that old
galaxies formed a plethora of little stars.
Our data provide the first observational confirmation of this effect, on scales
much larger that what had been observed to date for normal
galaxies,» adds Dominique Sluse of the Argelander - Institut für Astronomie in Bonn, Germany and University of Liège.
Dark matter's presence has for decades been inferred from its gravitational effects on
large - scale structures such as
galaxy clusters, but because it does not interact
much with ordinary matter and does not emit or absorb light — hence the «dark» moniker — it has so far proved impossible to observe firsthand.
Because protoclusters are spread out over a
much larger area of the sky, they are
much harder to find than
galaxy clusters.
Spiral
galaxies such as the Great Nebula in Andromeda are obvious candidates, but the elliptical
galaxies are
much older and more highly evolved and could conceivably harbor a
large number of extremely advanced civilizations.
Each magnified image makes the
galaxy appear as
much as 10 times
larger and brighter than it would look without the intervening lens.
«It's not where the star formation is, and to see so
much gas that far from the star - forming region means there is a
large amount of neutral hydrogen around the
galaxy,» Neeleman said.
The nursery is 6200 light years from the
galaxy's centre and spans 4400 light years, far
larger than any in the Milky Way, even though the
galaxy itself is
much smaller than ours.
Those theories suggest that, since there is
much more dark matter in the universe than visible matter,
galaxies will form where
large concentrations of dark matter (and hence stronger gravity) are present.
Dwarf
galaxies are sometimes embedded in a smoothly rotating disk of hydrogen gas that is
much larger than the
galaxy itself.
In such a model, the visible
galaxies ablaze in starlight are like the tip of an iceberg — the visible matter is at the very densest part of
much larger dark matter chunks.
This cluster has a diameter of approximately 15 million light years which is not
much larger than our Local Group but it contains fifty times the number of
galaxies.
Webb's giant sunshield will protect it from stray heat and light, while its
large mirror enables it to effectively capture infrared light, bringing us the clearest picture ever of space objects that emit this invisible radiation beyond the red end of the visible spectrum — early
galaxies, infant stars, clouds of gas and dust, and
much more.
The gas clouds in
galaxies are
much larger than the stars, so they will very likely hit the clouds in another
galaxy when the
galaxies collide.
@Amir: Too late too
much money is already been spent but you can explain the formation of
galaxies and overall
large scale structures of the material in the universe.
In 2003, the Anglo - Australian Observatory released a
much larger survey («2dF Galaxy Redshift Survey») of over 221,000
galaxies in two slices that extend over 1.5 billion light years in a two - degree field of the sky.
The
galaxies are
much fainter than the quasars so only the
largest telescopes can gather enough light to create a spectrum for those far away
galaxies.
NGC 3359 appears to be devouring a
much smaller gas rich dwarf
galaxy, nicknamed the Little Cub, which contains 10,000 times fewer stars than its
larger companion.
«The
galaxy we have observed, EGS8p7, which is unusually luminous, may be powered by a population of unusually hot stars, and it may have special properties that enabled it to create a
large bubble of ionized hydrogen
much earlier than is possible for more typical
galaxies at these times,» Sirio Belli, a Caltech graduate student who worked on the project, said, in the statement.
But astronomers also know that
much larger, supermassive black holes lie at the heart of
large galaxies including the Milky Way, where Sagittarius A * weighs as
much as 4 million suns.
Taking a closer look at the XDF (see a
larger version), there are lots of spiral
galaxies (similar to our own Milky Way), red
galaxies (the remnants of
galaxy collisions, which were
much more common when the universe had first formed), and tiny dots that are mere
galaxy seedlings.
Galaxies are
much larger systems of...
It may be that the
galaxy we have observed, EGSY8p7, which is unusually (intrinsically) luminous, has special properties that enabled it to create a
large bubble of ionized hydrogen
much earlier than is possible for more typical
galaxies at these times,» said Sirio Belli, a Caltech graduate student who helped undertake the key observations.
These are NGC4874 (right) and NGC4889 (left), they both have a diameter
larger than 250 000 light years and they are
much more massive than any
galaxies in the Virgo supercluster.
The amount of oxygen in a
galaxy is determined primarily by three factors: how
much oxygen comes from
large stars that end their lives violently in supernova explosions — a ubiquitous phenomenon in the early Universe, when the rate of stellar births was dramatically higher than the rate in the Universe today; how
much of that oxygen gets ejected from the
galaxy by so - called «super winds,» which propel oxygen and other interstellar gases out of
galaxies at hundreds of thousands of miles per hour; and how
much pristine gas enters the
galaxy from the intergalactic medium, which doesn't contain
much oxygen.
«But before we're ready to conduct a
large - scale survey of star - forming and starburst
galaxies with the SKA we need to know as
much as possible about these
galaxies and what triggers their extreme rate of star formation,» he said.
When the 300 - foot telescope observed
galaxies, it saw invisible gas extending farther out than the visible
galaxy — the
galaxy was
much larger than it appeared to optical telescopes.
But for observations of extremely dark
galaxies, we might need the Thirty Meter Telescope with
much larger light - gathering power.»
A
galaxy's core size typically is correlated to the dimensions of its host
galaxy, but in this case, the central region is
much larger than astronomers would expect for the
galaxy's size.
The researchers studied 72
large galaxy cluster collisions and found that, like
galaxies, the dark matter continued straight through the collisions without slowing down
much, meaning that dark matter do not interact with visible particles.
These filaments, spanning across millions of light - years —
much larger than the
largest galaxies — constitute the cosmic web, and account for most of the ordinary matter (as opposed to dark matter) in the universe.
The central bulge of M81 is home to significantly older stars, red in colour, and
much larger than the central bulge of our own
galaxy, the Milky Way.