Sentences with phrase «bright galaxy with»

Earth is inside a very bright galaxy with billions of stars and glowing gas.

J1415 +1320 is what's known as a blazar, a bright galaxy with a gluttonous supermassive black hole at its center (SN: 3/4/17, p. 13).

Therefore, evolutionist astronomers believe that star formation rates in our galaxy and nearby galaxies are too slow to be observed, but that amazingly high star formation rates occur in «starburst galaxies» — the brightest galaxies with the greatest redshifts.

Not exact matches

They are otherwise bright, talented people with a good product to offer, and yet, they lose this opportunity because they honestly believe that a being created the entire Universe and its billions of galaxies and then has a personal interest in their se.x lives.

Sky Sports reports that Christopher Samba is not the brightest star in the galaxy with his latest comments, claiming that Blackburn won't be relegated because they just have too much quality about them.

Hubble made an educated guess based on the reasoning that the brightest stars in each galaxy all shine with the same luminosity, like light bulbs of equal wattage, so the fainter they appear, the farther away they lie.

SLUGGISH STARS A hydrogen signature reveals the structure of six galaxies (top, bright regions appear red) observed with the Very Large Telescope in Chile.

The brighter regions correspond to the regions of the Universe with more galaxies and therefore more dark matter.

A barred spiral galaxy is a spiral galaxy with a band of bright stars emerging from the center and running across the middle of the galaxy.

Galaxies with more massive black holes turn out to have a higher concentration of stars in their central bulges, and consequently, the starlight is brighter in that region.

«This model is very intriguing with respect to one galaxy I've worked on a lot, which is particularly bright,» says Jacqueline Hodge of the Leiden Observatory in the Netherlands.

With five bright sources now confirmed, and more to follow, CR7 is now part of a unique «team» of bright early galaxies, suggesting there are tens to hundreds of thousands of similar sources in the entire visible Universe.

The galaxies — which would appear as flat, rotating disks — are brimming with extremely bright and massive blue stars.

Extremely bright exploding stars, called superluminous supernovae, and long gamma ray bursts also occur in this type of galaxy, he noted, and both are hypothesized to be associated with massive, highly magnetic and rapidly rotating neutron stars called magnetars.

The large, bright objects with spikes are stars in our own galaxy.

But the realization that quasars were really out at the edge of the observable universe, and thus must be far brighter than the brightest galaxy, posed a riddle that nobody has yet been able to answer with certainty: What are they?

At its peak, the burst slammed the telescope with 143,000 x-ray photons per second, making it the brightest x-ray burst ever seen beyond the Milky Way and its satellite galaxies.

Such a smash - up with a red giant would unleash much more energy than the decimation of a comet, so would have to occur in a distant galaxy to avoid appearing brighter than what was observed.

Using data from the Herschel Space Telescope, Negrello et al. (p. 800) showed that by searching for the brightest sources in a wide enough area in the sky it was possible to detect gravitationally lensed submillimeter galaxies with nearly full efficiency.

The Milky Way, the galaxy we live in, consists of a prominent, relatively flat disc with closely spaced bright stars, and a halo, a sphere of stars with a much lower density around it.

Some researchers theorized that these afterglows eluded detection because they occurred in a less dense region of a galaxy, where ejected material wouldn't have the opportunity to interact with lots of particles and produce a bright enough burst.

More than just Orion's brightest star, Rigel is among the most luminous objects in the galaxy, shining with the light of 55,000 suns.

Astronomers using the Subaru Telescope's Hyper Suprime - Cam observed the nearby large spiral galaxy M81, together with its two brightest neighbors.

Astronomers using the Subaru Telescope's Hyper Suprime - Cam prime - focus camera recently observed the nearby large spiral galaxy M81, together with its two brightest neighbors, M82 and NGC3077.

This galaxy is one of the brightest galaxies in the sky, and although it is too faint to see with the naked eye, it is an easy galaxy to find with binoculars if you know where to look.

The Subaru data reveal the presence of a surrounding large scale structure with the major axis running approximately north - west south - east (NW - SE), aligned with the cluster and its brightest galaxy shapes, showing elongation with a \ sim 2:1 axis ratio in the plane of the sky.

Paper and research team These observation results were published as Toba et al. «No sign of strong molecular gas outflow in an infrared - bright dust - obscured galaxy with strong ionized - gas outflow» in the Astrophysical Journal in December 2017.

M82 (left) is a very famous example of a starburst galaxy - it contains a lot of young, bright stars probably because a close encounter with its more massive neighbour M81 has triggered a lot of new star formation.

Like other spiral galaxies, the Milky Way Galaxy, has a bright disk of stars with sweeping arms of conspicously younger, brighter, and bluer stars enveloped in gas and dust that curve around its center like the arms of a huge pinwheel.

Messier 110 (M110, NGC 205) is the second brighter satellite galaxy of the Andromeda galaxy M31, together with M32, and thus a member of the Local Group.

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.

Astrophysics observations with K2 will include studies of young open clusters, bright stars, galaxies, supernovae, and asteroseismology.

A Seyfert galaxy is a spiral galaxy with a compact, very bright nucleus that produces a non-thermal continuous spectrum with broad (fat) emission lines on top.

NGC 55 is a bright, edge - on, irregular galaxy with a lot of new star formation.

With clouds shrouding much of the sky, professor Steve Fossey decided to point the University's 14 - inch telescope at nearby galaxy Messier 82 (M82) and saw a very bright object that wasn't supposed to be there.

It is an obvious group of galaxies because it contains several of the brightest galaxies in the sky (although they are all too faint to be seen with the naked eye).

The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions.

Webb will look for the bright objects that transformed this dark universe to the one we see today, ablaze with the glow of stars, gathered into immense galaxies.

With only a relatively minor change to the observing strategy, taking extra care to avoid extra glare from bright foreground light from the Earth, we enabled the Frontier Fields to see ever fainter and more distant galaxies than otherwise would have been possible.

Targeting bright giants, the method allows to obtain simultaneous age and chemical abundance information far deeper than would be possible with asteroseismology, extending the possible survey volume to remote regions of the Milky Way and even to neighbouring galaxies like Andromeda or the Magellanic Clouds already with present instrumentation, like VLT and Keck facilities.

All of the brightest and largest galaxies within 20 million light years are marked on this map together with many of the fainter dwarf galaxies.

In regards to this, Professor Ohta commented, «This is a big step towards getting the big picture of galaxy evolution as the objects connecting especially bright galaxies in millimeter / submillimeter waves and normal galaxies were detected with ALMA.»

Although GRB 000131, like other gamma - ray bursts, appears to have taken place in a remote «early galaxy» (or «sub-galactic clumps» of stars) that is smaller than today's luminous galaxies, astronomers found it difficult to detect that extremely dim, sub-galactic clump of stars even with the Hubble Space Telescope, as the observed fading of the afterglow indicated that the maximum brightness of the gamma - ray emission was explosion was at least 10,000 times brighter than its host galaxy.

New radio images of galaxies with bright quasar cores show that, though the galaxies appear normal in visible - light images, their gas has been disrupted by encounters with other galaxies.

For the first few days, you may notice some galaxies with unusually bright colors.

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.

Left - NGC 1313, a bright but rather isolated galaxy classified as a barred spiral galaxy (although with very short and irregular spiral arms).

Subsequently, however, an even more distant quasar with a tentative redshift of z = 6.40 was announced on January 9, 2003, near the SDSS detection limit of a redshift of z ~ 6.5 for bright quasars, and other teams of astronomers detected even more distant, fast - star - forming irregular proto - galaxies, including: gravitationally - lensed HCM 6A behind galaxy cluster Abell 370 with a redshift of z ~ 6.56, which appears to be converting about 40 Solar - masses into stars annually; (PhysicsWeb; IFA press release; Hu et al, 2002, in pdf; and erratum); and the possible «superwind - galaxy» LAE J1044 - 0130 (Subaru press release; and Ajiki et al, 2002, in pdf).

The galaxy hosts a bright quasar that may have illuminated the ghostly structure by hitting it with a beam of light from hot gas around a central black hole.

Young galaxies blaze with bright new stars forming at a rapid rate, but star formation eventually shuts down as a galaxy evolves.