NGC 6240 is an important object to investigate in order to understand the physical and evolutional relationship among the processes
of galaxy merger, the action of a starburst, and the phenomenon of an active galactic nucleus.
«These new observations help us put the pieces together by showing the first steps
of a galaxy merger in the early Universe.»
A successful detection would give astrophysicists a better understanding of the astrophysics at the hearts
of galaxy mergers, Mingarelli says, and provide a new avenue to study fundamental physics not accessible by any other means.
The team discovered the galaxy's peculiar features while conducting a Hubble survey of distant galaxies unleashing powerful blasts of radiation in the throes
of galaxy mergers.
Not exact matches
«The rate
of these neutron star
mergers in our
galaxy is about one every 100,000 years.
The scientists will now combine the results
of the Auriga Project work with data in surveys from observatories like the Gaia mission, to better understand how
mergers and collisions shaped
galaxies like our own.
Many other potential applications
of this dataset are explored in the series
of papers, and they include studying the role
of faint
galaxies during cosmic reionisation (starting just 380,000 years after the Big Bang),
galaxy merger rates when the Universe was young, galactic winds, star formation as well as mapping the motions
of stars in the early Universe.
The team think a
merger of galaxies is driving star formation, «but we do not yet understand the physics», says Swinbank.
The detection
of a supermassive black hole
merger would offer new insights into how massive
galaxies and black holes evolve, Mingarelli says.
One surprise from the results was which
galaxies are most likely to offer the first glimpse
of supermassive black hole
merger.
Such
mergers could give themselves away by their effect on the shapes
of the black holes» parent
galaxies, and in infrared and ultraviolet afterglows.
«Galaxy
mergers are common, and we think there are many
galaxies harboring binary supermassive black holes that we should be able to detect,» said Joseph Lazio, one
of Taylor's co-authors, also based at JPL.
«
Galaxies are shaped by collisions and
mergers, as well as this sweeping
of their gas from cosmic winds.
Because these events unfold on billion - year timescales, each pair
of galaxies observed by Hubble provides just a snapshot at a particular stage
of the collision and
merger process.
Simulations
of galaxy formation suggest that such bright
galaxy mergers could form, but not in the numbers seen during that active epoch.
These superbright submillimeter
galaxies, they decided, must also be the result
of mergers.
Astronomers speculate that this
merger may eventually form the core
of an entire
galaxy cluster.
Over billions
of years, these
mergers continued, eventually producing the large
galaxies and clusters
of galaxies we see in the Universe today.
The sharp - eyed Hubble is offering support for the fertile
merger of spiral
galaxies.
SPD.81 may be a rotating disk
of stars seen edge on, the team suggests, or it could be the result
of the
merger of two smaller
galaxies.
Lee thinks the
galaxy probably formed not from the cataclysmic collapse
of one big gas cloud but from the
mergers of many smaller ones.
«These results are powerful evidence that a significant
galaxy evolution has taken place throughout the universe's history, which dramatically reduced the number
of galaxies through
mergers between them — thus reducing their total number.
These results contribute new information to the studies
of galaxy evolution and its relation to
galaxy -
galaxy mergers.
Stellar motions in the core
of the giant
galaxy do indeed suggest that it may have experienced a black hole
merger in the not - too - distant past, says Gebhardt.
Today most
galaxies show signs
of past
mergers and near - collisions.
At the same time, the gas in the
galaxy disks loses its angular momentum via viscous process associated with gas mixture, and falls into the gravitational center
of the
merger.
Astronomers think that the
galaxy merger process
of NGC 6240 began about a billion years ago, so this work suggests that the later stages
of the
merger are what excited the gigantic starbursts and subsequent superwinds.
To identify the final shapes
of galaxies after
mergers observationally, the group studied the distribution
of gas in 37
galaxies that are in their final stages
of merging.
For decades scientists have believed that
galaxy mergers usually result in the formation
of elliptical
galaxies.
Supermassive black holes like the one in
galaxy M87 probably grow not only by feeding on infalling gas and stars but also by
mergers of smaller black holes.
«A violent wind blown from the heart
of a
galaxy tells the tale
of a
merger.»
Those other processes include collisions
of giant gas clouds within
galaxies, internal instabilities, tidal interactions during flybys
of smaller
galaxies, and minor
mergers that don't produce conspicuous distortions.
The thought was that when many
galaxies are close together, a
merger, two
galaxies colliding and melding together, would create instabilities and cause gas to fall into the super massive black hole in one
of the
galaxies, creating a quasar.
The Hubble data indicate that they are «wobbling» around the centre
of mass
of each cluster long after the
galaxy cluster has returned to a relaxed state following a
merger.
«We've known for awhile that minor
mergers can have visible effects on their host
galaxies,» says David Law, an astrophysicist at the University
of Toronto's Dunlap Institute for Astronomy and Astrophysics, who did not contribute to the new study.
Comparing that
galaxy's redshift with the distance
of the
merger as measured by the loudness
of the gravitational waves could provide an independent estimate
of the rate
of cosmic expansion, possibly more accurate than current methods.
But new observations by Herschel, a far infrared space observatory operated by the European Space Agency, show that massive elliptical
galaxies can form from the
merger of two large
galaxies.
The most plausible explanation for this propulsive energy is that the monster object was given a kick by gravitational waves unleashed by the
merger of two hefty black holes at the center
of the host
galaxy.
Conroy suspects that violent conditions in the early universe — such as
galaxy mergers — shocked and compressed gas and dust in particular areas, creating agglomerations
of thousands
of stars in particular areas.
Perhaps, after all, a relatively recent galactic
merger is responsible for Andromeda's structure — and the structure
of countless other
galaxies — as well.
By comparing the models to recent observations
of clusters in the Milky Way
galaxy and beyond, the results show that Advanced LIGO (Laser Interferometer Gravitational - Wave Observatory) could eventually see more than 100 binary black hole
mergers per year.
If you wait long enough, the cluster
mergers make the
galaxies even more red and dead — they slip back into a coma and have little prospect
of a second resurrection.»
The unprecedented deep image
of the
galaxy reveals evidence
of a hidden minor
merger billions
of years ago.
The new work implies that the
merger of galaxy clusters has a major impact on the formation
of stars.
Dr. Masafumi Yagi, who leads the next phase
of the project said, «We will discover more and more evidences
of the satellite
merger around Seyfert host
galaxies.
Does the image appear to depict a
merger of multiple
galaxies?
It's a different story with dwarf
galaxies: they often hang out at the fringes
of larger
galaxies, whose gravity strips them
of their stars before a
merger can take place.
Clusters grow through the accretion
of gas from these large - scale filaments and through
mergers with other clusters and groups
of galaxies.
A new study has come to the startling conclusion that as many as half
of all stars in the universe may be rogue, having been ejected from their birthplaces by
galaxy collisions or
mergers.
If
galaxies that have never been through a
merger, like NGC 4178 — detectable by their lack
of stellar bulges — have their own central black holes, their properties could help tell the story.