Sentences with phrase «galaxy at»

Samsung is all set to launch the next galaxy at unpacked event, but hours before official launch multiple photos of galaxy S5 has been leaked.

After your first mission you will be afforded the ability to explore the galaxy at your own whim.

Even if there is a nice twist, it's not totally unexpected, and it can usually be predicted that your character will play a side role in whatever conflict is happening in the galaxy at large.

Explore the galaxy at a more leisurely pace or throw your controller across the room in frustration — the choice is up to you!

This is a galaxy at war and it will be up to you to choose your role.

• Three New Maps — With the fate of the galaxy at stake, Earth's military efforts have concentrated on three strategic locations.

Still, while the movie does flip all across the galaxy at a moment's notice, it doesn't flip too fast.

And «slightly» is important — a big part of the fun is watching Chris Pratt deliver the type of performance that you'd hire Chris Pratt for, albeit in epic space battles with the fate of the galaxy at stake.

However, there's no way she would sit out a fight that literally has the fate of the galaxy at stake.

When a sufficient amount of dark matter has gathered, it attracts ordinary matter (mostly hydrogen and helium gas) to form stars that may eventually form a luminous galaxy at the core.

Each clump has brightness comparable to a typical luminous galaxy at the epoch of Himiko, when the Universe was only 800 million years old.

ESA says Gaia will map 1 percent of the stellar content in the Milky Way, which puts the estimate of the total stars in our galaxy at 100 billion.

The color renders the strength of UV emission by triply ionized Carbon (C IV) in the CGM gas surrounding a Milky - Way - analog galaxy at z ~ 0.25.

«The surprising aspect about the present discovery is that we have detected this Lyman - alpha line in an apparently faint galaxy at a redshift of 8.68, corresponding to a time when the Universe should be full of absorbing hydrogen clouds,» said co-author and Caltech astronomer Richard Ellis.

Dwingeloo 1 (right) is a barred spiral galaxy at the back of the group but it is so faint that it was not discovered until 1994.

Figure 2 Artist impression of galaxy at the center of the Phoenix Cluster.

«The surprising aspect about the present discovery is that we have detected this Lyman - alpha line in an apparently faint galaxy at a redshift of 8.68, corresponding to a time when the universe should be full of absorbing hydrogen clouds,» Richard Ellis, a former faculty member of the California Institute of Technology, and co-author of a paper detailing the findings, published in the Astrophysical Journal Letters, said in a statement.

The density - wave theory, proposed by Frank Shu and C.C. Lin in 1964, says that a galaxy's spiral pattern is a wave of higher density, or compression, that revolves around the galaxy at a speed different from that of the galaxy's gas and stars.

That is, if you can see the galaxy at all.

Eight bright X-ray sources located far beyond the galaxy at distances of hundreds of millions of light - years were observed with Chandra, which revealed that the X-rays from these distant sources are absorbed selectively by oxygen ions in the vicinity of our galaxy.

By measuring this stretch, one can calculate how long the light's journey has taken, and place each galaxy at the right point in cosmic history.

Some 90 years later, we know that M31 is about 2.5 million light - years away, and is approaching our galaxy at about 109 km / sec.

M87 (bottom - left) is the very large and active galaxy at the centre of the Virgo cluster.

In the same field of view is NGC 4647 - a spiral galaxy at a different distance.

NGC 4697 (centre) is the large bright elliptical galaxy at the centre of the NGC 4697 group.

NGC 1399 (centre) is the large elliptical galaxy at the heart of the cluster.

Using the precise VLA position, researchers used the Gemini North telescope in Hawaii to make a visible - light image that identified a faint dwarf galaxy at the location of the bursts.

Follow - up spectroscopy with the IMACS instrument on the 6.5 m Magellan Baade telescope confirms one of these as a z = 1.975 quasar quadruply lensed by a double galaxy at z = 0.293.

Astronomers have clocked a black hole racing through the flattened disk of the Milky Way galaxy at 400,000 kilometers per hour.

The monster, for its part, is in direct contact with only a fairly small neighborhood and should be oblivious to what happens in the galaxy at large.

The survey has turned up several galaxies so small and faint that they challenge the definition of what counts as a galaxy at all.

«A galaxy at its very early stages of life, full of dust and gas, has a very high star formation rate but at the same time it still contains very few stars because it hasn't had the time to form them yet, that's all.»

«We see some gas outflowing from this galaxy at millions of miles per hour, and this gas may have been blown away by the powerful radiation from the newly formed stars,» said Ryan Hickox, an astrophysicist at Dartmouth College, Hanover, N.H., and a co-author on the study.

What looks like a celestial hummingbird is really the result of a collision between a spiral and an elliptical galaxy at a whopping 326 million light - years away.

A small number of stars moving so fast they'll eventually escape the Milky Way may not have come from our galaxy at all.

Our entire galaxy rushes toward the Andromeda galaxy at 80 miles per second.

Colleagues were startled that Spitzer saw the galaxy at all.

In the kind of explosion that leaves behind a neutron star, this star recoils and careens across the galaxy at high speed.

This neutrino jet can kick pulsars across the galaxy at speeds of several hundred miles per second.

Here, we report on a ~ 200 - second x-ray quasi-periodicity around a previously dormant SMBH located in the center of a galaxy at redshift z = 0.3534.

Image of the gravitational lens RX J1131 - 1231 galaxy with the lens galaxy at the center and four lensed background quasars.

Instead, van Dokkum's team found those star clusters moving languidly around NGC 1052 - DF2, a sign that there may well be very little or no dark matter within that galaxy at all.

The fantastic sensitivity of the VLA allowed the researchers to monitor the radio galaxy at the necessary cadence without having to disrupt the observatory's regular schedule of operations.

GLOWING GAS Hanny's Voorwerp, the greenish smudge at the left of this image, is glowing thanks to photons from a feasting black hole in the galaxy at right.

Likewise, our sun — and every other star in the sky — accelerates toward the center of the Milky Way galaxy at a rate that works out to about the width of an atom per second every second.

It's the brightest known galaxy at that distance.

In the Fornax cluster (right) the core cloud is swept back like a comet's tail toward the top of the image, indicating it is moving through even more diffuse gas on a collision course with the galaxy at lower left.

By peering this deeply into the galaxy at millions of stars, astronomers should unleash «a tsunami of transit discoveries» within the next several years, Sasselov predicts.

The innocuous - looking spiral galaxy at bottom left (lower left corner) illustrates the power of dark matter.

This is an artist impression of galaxy at the center of the Phoenix Cluster.