Here are images of six different
galaxy clusters taken with NASA's Hubble Space Telescope (blue) and Chandra X-ray Observatory (pink) in a study of how dark matter in clusters of galaxies behaves when the clusters collide.
Zitrin's team spotted the galaxy's gravitationally multiplied images using near - infrared and visible - light photos of
the galaxy cluster taken by Hubble's Wide Field Camera 3 and Advanced Camera for Surveys.
Work on infrared studies of local
galaxy clusters took me to the International Science and Engineering Fair (ISEF) in 2007 where I won the Bok Second Prize.
Not exact matches
The light from the exploding star, which
took 9.4 billion years to reach Earth, fell squarely on one
galaxy sitting in one of the Frontier Fields
clusters.
The massive
galaxy cluster Abell 2744, nicknamed Pandora's Cluster, takes on a ghostly look in this Hubble Space Telescope view where the total starlight from the cluster has been artificially colore
cluster Abell 2744, nicknamed Pandora's
Cluster, takes on a ghostly look in this Hubble Space Telescope view where the total starlight from the cluster has been artificially colore
Cluster,
takes on a ghostly look in this Hubble Space Telescope view where the total starlight from the
cluster has been artificially colore
cluster has been artificially colored blue.
Perhaps only when we study huge agglomerations of matter, in
galaxies or
clusters of
galaxies, will we spot the elusive phenomena that can
take us beyond Einstein and Newton.
In a paper to appear in Publications of the Astronomical Society of Australia, Forbes and Kroupa have offered five possible criteria for determining whether an object is a
galaxy: the presence of dark matter, multiple generations of stars, satellite star
clusters, a minimum size, and the time it
takes for gravitational interactions between stars to slow them all down to roughly the same speed.
It is what holds together giant
clusters of
galaxies, but it is also what I experience every time I sit down in a chair or
take a step.
Using the Hubble Space Telescope, the international team of collaborators peered across cosmic time to observe 65 distant
galaxy clusters whose light has
taken billions of years to reach Earth.
Among the stunning shots
taken this week were those of the Lagoon Nebula, about 3600 light years away from Earth; the 47 Tucanae
cluster of several million ancient stars about 15,000 light years from Earth; and the face - on barred spiral
galaxy NGC 6744 in the star - rich southern constellation of Pavo, about 30 million light years away.
To make these discoveries, the team utilised the deepest images of gravitational lensing made so far in three
galaxy clusters, which were
taken as part of the Hubble Frontier Fields programme [4].
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.
Gravitational lensing happens when huge collections of matter — such as those found in
galaxy clusters — warp the space - time around them so that the light from objects behind the
clusters takes a curved path.
An image
taken with the Hubble Space Telescope of Abell 1689, a massive
cluster of
galaxies whose gravitational pull is so strong that it bends light, acting like a lens.
Oliver Tunnah, a regular user of the FTs
took this great image of the distant
galaxy cluster Abell 2065 during one session on FTS.
15 Moreover, fully formed
clusters of
galaxies, not just
galaxies, are seen at the greatest distances visible to the Hubble Space Telescope.16 In 1998 and 2004, similar pictures — with similar results — were
taken.
Abstract: We derive an accurate mass distribution of the
galaxy cluster MACS J1206.2 - 0847 (z = 0.439) from a combined weak - lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
cluster MACS J1206.2 - 0847 (z = 0.439) from a combined weak - lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations
taken as part of the
Cluster Lensing And Supernova survey with Hubble (CLASH) p
Cluster Lensing And Supernova survey with Hubble (CLASH) program.
We find good agreement in the regions of ove... ▽ More We derive an accurate mass distribution of the
galaxy cluster MACS J1206.2 - 0847 (z = 0.439) from a combined weak - lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) p
cluster MACS J1206.2 - 0847 (z = 0.439) from a combined weak - lensing distortion, magnification, and strong - lensing analysis of wide - field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations
taken as part of the
Cluster Lensing And Supernova survey with Hubble (CLASH) p
Cluster Lensing And Supernova survey with Hubble (CLASH) program.
In addition, the latest discovery also indicates that much of the star formation in these
galaxies takes place after the
galaxies fall onto the
cluster.
No one had
taken ultra-deep images of a
galaxy cluster with Hubble or Spitzer.
This image of
galaxy cluster Abell 2744, also called Pandora's Cluster, was taken by the Spitzer Space Tel
cluster Abell 2744, also called Pandora's
Cluster, was taken by the Spitzer Space Tel
Cluster, was
taken by the Spitzer Space Telescope.
The high - resolution images
taken by the Hubble Space Telescope for the Frontier Fields survey have yielded a treasure trove of insights into very distant
galaxy clusters.
What if we could
take a well - known
galaxy and put it behind one of our Frontier Fields
galaxy clusters?
On June 16, 2010, the Hubble Heritage Project released a very detailed, composite image of the dark lanes of dust crisscrossing the giant elliptical
galaxy Centaurus A.
Taken on July 10, 2010 with the Hubble Space Telescope's Wide Field Camera 3, the panchromatic image of ultraviolet through near - infrared wavelengths shows new details such as bluish
clusters of young massive stars and reddish gas nebulae undergoing star birth normally obscured by dust.