This would be an early phase of strong environmental effects seen in
the present galaxy clusters.
Not exact matches
As it has countless times in the past and
present, (the Holocaust, the Bubonic Plague, the World Wars, countless natural disasters, (floods, storms, earthquakes, etc), the Sky Myth was on vacation when, on a tiny speck of a planet, on a boring arm of the
galaxy, in an average
galaxy cluster among billions, a bad thing happened.
In the bottom box is a reconstructed image, based on modeling, that shows what the
galaxy would look like if the
galaxy cluster were not
present.
Among other things, the new map will help astronomers to understand and explain the motion of the Milky Way, which is apparently being tugged by the gravity of neighboring groups and
clusters of
galaxies, says 2MASS team member Karen Masters of the University of Portsmouth in the United Kingdom, who
presented the it here at the summer meeting of the American Astronomical Society.
A striking image
presented here 3 June at the meeting of the American Astronomical Society shows a globular
cluster known as Palomar 5 being torn asunder by tidal forces of our home
galaxy.
To determine how and why
clusters formed, it is critical to investigate not only mature
galaxy clusters as seen in the
present Universe but also observe protoclusters,
galaxy clusters in the process of forming.
Both the COBE ripples and the large - scale
clustering of
galaxies can be explained by a CDM universe in which 80 per cent of the
present mass density is contributed by a cosmological constant, though some cosmologists argue that such theories may not explain the motions of
galaxies.
At
present it makes itself felt only over huge distances, such as the gaps between
clusters of
galaxies, but Caldwell says that some theories indicate that dark energy might just be kicking into gear.
Some ellipticals are
present in the central part of the
cluster including a giant elliptical at the center (M87) that has become so large by gobbling up nearby
galaxies that were attracted by its enormous gravity.
This statement is certainly true if we assume that the only gravitational force
present is that exerted by visible matter, but it is true even if we assume that every
galaxy in the
cluster, like the Milky Way, is surrounded by a halo of dark matter that contains 90 percent of the mass of the
galaxy.»
It is thus an example of a progenitor or ancestor of a
present - day
galaxy cluster, or proto -
cluster for short.
The newly discovered «proto -
cluster» of
galaxies, observed when the universe was only 1.7 billion years old (12 percent of its
present age), is one of the most massive structures known at that distance.
Galaxy
clusters are commonly observed in the
present - day universe and contain some of the oldest and most massive
galaxies known.
Dr. Jean Brodie, from the University of California at Santa Cruz, will trace the formation and evolution of
galaxies over cosmic time, making use of some «astronomical fossils» called globular star
clusters, that are bright beacons tracing all the mergers and acquisitions that have assembled into
present day
galaxies.
«We
present results from an optical - infrared photometric study of early - type (E+S 0)
galaxies in 19
galaxy clusters out to z = 0.9.»
SDSS studies have probed the dark matter environments of quasars through
clustering measurements, revealed populations of quasars whose central engines are hidden by obscuring dust, captured changes in quasar spectra that show clouds moving in the gravitational grip of the central black hole, and allowed a comprehensive census of the much fainter accreting black holes (active galactic nuclei, or AGN) in
present - day
galaxies.
In the adjacent gallery, Thater
presents Visual Voyage: Milky Way to the Virgo
Cluster (2015) and Aquarius Halos (2015), two videos of stars and
galaxies swirling and advancing toward the viewer.