Now Andrew Gould and Jens Villumsen of Ohio State University in Columbus argue that the gravity of
nearby galaxy clusters should distort the light from distant galaxies in a way that depends on W.
Astronomers first noticed some years ago
that nearby galaxy clusters are populated with dim reddish elliptical galaxies.
However, if the light from many distant galaxies passes through the stretched spacetime of
a nearby galaxy cluster, then the mass of the galaxy cluster can be derived from a careful analysis of the ensemble of warped shapes and their orientations.
Not exact matches
A Giant Galactic Ghost Intrigued by faint blurs on old photographic plates of the Virgo
galaxy cluster, a
nearby region teeming with
galaxies, Oregon's Bothun and colleagues wondered if the apparitions might be smallish
galaxies with «low surface brightness» — astronomer - speak for emitting less light per unit area than typical
galaxies.
Gas at the centre of
galaxy clusters should be cooling as it loses energy; this would allow
nearby material to compress the gas and create ideal conditions for making stars.
The globular
clusters M15 (left) in our Milky Way and G1 in the
nearby Andromeda
galaxy both harbor medium - size black holes at their cores.
Now, Hubble has done just that for two globular
clusters: M15, in our Milky Way, and G1, in the
nearby Andromeda
galaxy.
By studying this particular
cluster — and others
nearby — astronomers can explore the properties of the spiral disc of our
galaxy, the Milky Way.
He notes that the Milky Way's north side points toward the Virgo
cluster, an enormous
nearby gathering of
galaxies.
THE distance to the
nearby Virgo
cluster of
galaxies is a crucial measurement.
The astronomers believe that AzTEC - 3 and the other
nearby galaxies appear to be part of the same system, but are not yet gravitationally bound into a clearly defined
cluster.
If they are connected gravitationally, then they will eventually form the core of a massive
cluster of galaxies like the nearby Virgo Cluster, which boasts 2000 m
cluster of
galaxies like the
nearby Virgo
Cluster, which boasts 2000 m
Cluster, which boasts 2000 members.
Lauer and his colleagues began their survey of
galaxy clusters in order to find the «great attractor», a concentrated mass supposedly responsible for the net motion of
nearby galaxies.
Remarkably, the distribution of star - forming
galaxies around a
cluster of
galaxies in the more distant universe (5 billion years ago) corresponds much more closely with the weak lensing map than a slice of the more
nearby universe (3 billion years ago).
The lens could lie within or
nearby the
galaxy, and could be a collection of thousands of stars like a globular
cluster.
These rare systems — only a few tens were known until recently — were thought to have had their outer coats of stars ripped away by the gravity of other, larger
galaxies as they passed
nearby, a theory supported by the fact that they were usually found in the centers of large
clusters of
galaxies.
Gravitational lenses occur when very massive objects — such as
clusters of
galaxies — warp spacetime around them, causing light (and anything else) traveling
nearby to take a curved path.
The greater W is, the more mass these
nearby clusters have and the more their gravity should distort, or «lens», the light from
galaxies behind them.
These
nearby objects include the Local Supercluster, a vast assemblage of
galaxies to which our
Galaxy, the Milky Way, belongs and the coma
cluster, a
galaxy cluster that lies a few hundred million light years away in the constellation of Coma Berenices.
First, the
cluster is
nearby, so its
galaxies are bright and many of them have measured velocities.
Seeing these seven
clusters fairly
nearby suggests our theories of how
galaxies form via collisions are right.
In reality, NGC 1559 is physically nowhere near the LMC in space — in fact, it truly is a loner, lacking the company of any
nearby galaxies or membership of any
galaxy cluster.
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.
Figure 1 shows a
nearby galaxy surrounded by globular
clusters.
Gillian Wilson, professor of physics and astronomy at UC Riverside, added, «Fascinatingly, however, the study found that the percentage of
galaxies which had stopped forming stars in those young, distant
clusters, was much lower than the percentage found in much older,
nearby clusters.
A
nearby companion
galaxy, NGC 5195, off the edge of this image, gravitational pull is triggering star formation in the main
galaxy, as seen in brilliant detail by numerous, luminous
clusters of young and energetic stars.
His scientific research has focused on dwarf spheroidal
galaxies, stellar populations in the Milky Way
galaxy and
nearby galaxies, globular
clusters, chemical evolution of
galaxies, and dark matter.
The protocluster is likely to evolve, over 12 billion years, into a system much like the
nearby Coma
cluster of
galaxies, shown in the image below.
These structures can be traced over more than 80 million light - years in the COSMOS survey - approximately five times the extent of the
nearby Virgo
galaxy cluster.
Astronomers reported today that recent ultraviolet observations with NASA's Hubble Space Telescope suggest that what were thought to be randomly distributed,
nearby primordial clouds of hydrogen may actually be associated with
galaxies or
clusters of
galaxies.