Not exact matches
those stars you see, the light takes hundreds of thousands of years to reach us, and when you see that light from them, you are seeing what they looked like thousands of years ago when that
group of photons was thrust out
by that star /
galaxy, which than takes several light years to reach us, which also means you are looking at the past, thousands and hundreds of thousand of years into the past!
Instead, van Dokkum found his
galaxies by grouping eight 400 - millimeter lenses into a contraption resembling an insect's compound eye.
Now a
group of astronomers led
by Asa Bluck of the University of Victoria in Canada have found a (relatively) simple relationship between the colour of a
galaxy and the size of its bulge: the more massive the bulge the redder the
galaxy.
MOST stars are gregarious,
grouping together
by the billions in
galaxies like our Milky Way.
They appear to be caused
by mysterious events beyond our Milky Way Galaxy, and possibly even beyond the Local
Group of
galaxies that includes the Milky Way.
Most of the universes»
galaxies, which each contain billions of stars, are surrounded
by up to several thousands of so - called globular clusters,
groups of up to a million suns packed into dense spheres
by gravity.
To locate the source, a
group directed
by Puget and David L. Clements in Paris has started the first far - infrared search for distant
galaxies, using the European Space Agency's Infrared Space Observatory (ISO).
Visible light (second inset) shows a vast, elliptical
grouping of stars bisected
by a dark lane of dust, which astronomers interpret as the remains of a spiral
galaxy that collided with a larger elliptical
galaxy.
The 2dF
group aims to measure the speeds of 250,000
galaxies by the end of 2001, and the mass estimates will improve with more data, Dalton notes.
One, a
group of Fermi researchers led
by Johann Cohen - Tanugi of Montpellier University in France and Jan Conrad and Maja Llena Garde, both of Stockholm University in Sweden, looked at two years» worth of observations of 10 dwarf
galaxies.
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.
Dynamical analysis for nonisolated
galaxies demonstrates the feasibility of their ejection from host clusters and
groups by three - body encounters, which is in agreement with numerical simulations.
Those remnants, which McConnachie calls «the partially digested remains of these dwarf
galaxies,» take the form of large, diffuse streams of stars, former galactic
groupings that have been pulled apart
by the larger
galaxy's gravitational pull.
Left, a
group of
galaxies mapped
by KiDS.
An international team of astronomers led
by the Max Planck Institute for Astronomy (MPIA) has made a surprising discovery about the birthplace of
groups of stars located in the halo of our Milky Way
galaxy.
«We showed that it may be fairly common for
groups of stars in the disk to be relocated to more distant realms within the Milky Way — having been «kicked out»
by an invading satellite
galaxy.
These «ultra-compact dwarf
galaxies» are now the second and third ones known to house such gargantuan black holes, confirming that the first one — discovered
by the same
group in 2014 — was not an anomaly.
Maunakea, Hawaii — An international team of astronomers led
by the Max Planck Institute for Astronomy (MPIA) has made a surprising discovery about the birthplace of
groups of stars located in the halo of our Milky Way
galaxy.
Holmberg II (right) is one of nine low - surface - brightness
galaxies listed
by Erik Holmberg in the 1950's, three of which are associated with the M81
group.
In 1986 a
group of astronomers observing the motions of the Milky Way and neighbouring
galaxies noted that the
galaxies were moving toward the Hydra - Centaurus superclusters in the southern sky with velocities significantly different from those predicted
by the expansion of the universe in accordance with the Hubble law (see Hubble's constant).
Galaxies are classified or
grouped by their shape.
This discovery of this system is part of a large survey for quasar sightlines which pass near
galaxies, which is coordinated
by Joseph Hennawi, the leader of theENIGMA research
group at the Max Planck Institute for Astronomy.
On the evening of July 3, 2014, both of the mighty 10 - meter Keck Observatory telescopes were steered
by Dr. Andrea Ghez and her team of observers from the UCLA Galactic Center
Group to study the supermassive black hole at the center of our
galaxy.
This simulation shown here was run
by the Making
Galaxies in a Cosmological Context (MaGICC) project in the theory
group at MPIA.
Since low - mass stars like GJ 1132 are among the most common in the
galaxy and are known to host
groups of small planets, the researchers said that they are encouraged
by their discovery and the possibility that such worlds could maintain atmospheres despite the high levels of activity in and around such stars.
A lot of the
galaxies in this
group lie directly behind the plane of our
galaxy and are hidden
by all the intervening gas, dust and stars.
The
grouping of these
galaxies around the Milky Way Galaxy is mimicked in the case of the Andromeda Galaxy, which is also accompanied
by several dwarf companions.
However, new work
by astronomers at the University of Sheffield has discovered an incident of a star being destroyed
by a supermassive black hole in a much smaller sample size — a
group of just 15
galaxies.
The Milky Way system is near one end of the volume of space occupied
by the Local
Group, and the great Andromeda
galaxy (M31) is near the other end, about 2,000,000 light - years away.
MAUNAKEA, Hawaii — A
group of researchers, led
by a University of California, Riverside graduate student, observed distant
galaxies with the MOSFIRE high - resolution near - infrared spectrometer at W. M. Keck Observatory and their results will help to build the foundations of
galaxy evolution studies
by predicting the star - formation rate of distant
galaxies from the light they emit.
This cluster completely dominates our tiny corner of the Universe, and even our Local
Group of
galaxies is being gravitationally pulled
by this cluster.
Examples of science projects enabled
by the data in the High - Latitude Survey include: mapping the formation of cosmic structure in the first billion years after the Big Bang via the detection and characterization of over 10,000
galaxies at z > 8; finding over 2,000 QSOs at z > 7; quantifying the distribution of dark matter on intermediate and large scales through lensing in clusters and in the field; identifying the most extreme star - forming
galaxies and shock - dominated systems at 1 < z < 2; carrying out a complete census of star - forming
galaxies and the faint end of the QSO luminosity function at z ~ 2, including their contribution to the ionizing radiation; and determining the kinematics of stellar streams in the Local
Group through proper motions.
An international
group of scientists led
by German Hans - Walter Rix from the Max - Planck - Institut fur Astronomie in Heidelberg is studying 24 nearby disk
galaxies, similar to our own Milky Way, using the NASA / ESA Hubble Space Telescope.
Some of these
galaxies still have uncertain distances, especially the Maffei
group galaxies and also some
galaxies in the far southern hemisphere which can not be seen
by Russian telescopes.
The Sculptor
group is the nearest group of galaxies to the Local Group and is dominated by five galaxies, four spiral - NGC 247, 253, 300 and 7793 and one irregular - NG
group is the nearest
group of galaxies to the Local Group and is dominated by five galaxies, four spiral - NGC 247, 253, 300 and 7793 and one irregular - NG
group of
galaxies to the Local
Group and is dominated by five galaxies, four spiral - NGC 247, 253, 300 and 7793 and one irregular - NG
Group and is dominated
by five
galaxies, four spiral - NGC 247, 253, 300 and 7793 and one irregular - NGC 55.
In the paper, the
group of researchers, led
by Irene Shivaei, observed 17 bright distant
galaxies with the MOSFIRE high - resolution near - infrared spectrometer at the W. M. Keck Observatory telescopes.
The as - yet untitled Star Wars standalone movie, heavily rumoured to follow a
group of bounty hunters around the
galaxy, has been gaining traction of late; Gary Whitta, the movie's original writer, left the project, while Simon Kinberg (X-Men: Days of Future Past, Star Wars Rebels) has joined The Empire Strikes Back scribe Lawrence Kasdan for the second standalone film, which will be directed
by Josh Trank (Chronicle).
She is joined
by a pair of Force - sensitive monks (Donnie Yen and Jiang Wen) and a sarcastic reprogrammed Imperial robot, K - 2SO (Alan Tudyk), as this motley
group tries to verify the message and potentially work even at odds with the Rebel Alliance to save the
galaxy from tyranny.
Then I discovered Dust a FREE FPS, sure it was rough around the edges during beta and before the Uprising update, but a game that's more in depth, that rewards you for being more tactical than foolish and also lets you drive tanks, pilot drop ships or call in bombardments from space... all in the context of an ever changing
galaxy with planets up for grabs
by groups of players known as corporations.
Take part on your mobile device and decide the fate of the
galaxy's bumbling defenders
by voting on each crucial decision as a
group, for better or worse.
A new
group show at Kopeikin Gallery organized
by Katie Shapiro and Sean Higgins explores the idea of the «transporter» as used in science fiction — the object or device that allow people to travel from one side of the
galaxy to the other.
This image made
by the NASA / ESA Hubble Space Telescope shows part of a
group of five
galaxies known as Stephan's Quintet.
While large Beltway environmental
groups support it, a
galaxy of smaller ones say the House bill has been mortally weakened
by giveaways just getting out of its first committee.