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词汇 example_english_galaxy
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Examples of galaxy


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Nevertheless, galaxies with highly peculiar morphological properties were found by us during our searches, and will be investigated in detail in the years to come.
When we turn from galaxies to the distribution of galaxies, the distribution does not seem to exhibit design - it looks rather random and haphazard.
On the outside of galaxies there is much less light, meaning that there is much less mass concentrated in these regions.
The interactions of galaxies will also lead to large changes of angular momentum and energy.
Research on barred galaxies has been performed using observations, theory and numerical simulations.
We have never observed galaxies in the process of controlled disintegration.
Following the introductory chapter, the next section reviews the current state of cosmology and prevalent theories of how matter, stars, galaxies and the universe formed.
I have distinguished three sorts of galaxies, but it remains an open question which of the three types are instantiated.
Quasars are widely believed to be the cores of young galaxies.
Such a regime may hold at the centre of galaxies or close to collapsed stars.
Perhaps the strongest form of evidence for the existence of dark matter is the rotation curves of galaxies.
There must have been something there to contribute to the gravity needed to keep the stars and galaxies gravitationally bound to their system.
Such a large axion density would be incompatible with the formation of galaxies and so is anthropically disallowed.
We read how the galaxies are grouped in clusters.
The possibility of this happening is about as likely as humans walking the surface of planets of distant galaxies.
Change was a given, inducing gradients, forming systems and evolving structures, and the results, emergent over billions of years, included galaxies, stars, planets and life.
Examples of systems are water molecules, galaxies, and babies.
The two most common types of galaxies are globular galaxies and spiral galaxies.
Essentially this means that surveys of deep space could be showing us multiple images of the same finite set of galaxies - this is like being in a hall of mirrors.
If galaxies themselves were like kinetic sculptures, or if they were arranged with each other like kinetic sculptures, this would be confirmation of design - but the apparent chaos is not.
The main challenge here is to find out how these galaxies manage to convert so much gas into stars so efficiently and in such a very short time.
In the same way, they can contribute to our developing understanding of phenomena associated with other galaxies.
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Here we are, microscopic creatures scuttling about on the surface of a minor planet circling round a second-rate star in one of halt-a-million galaxies.
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Well, for years, amateur astronomers have made important contributions to professional astronomy, spotting comets and supernovae, and monitoring exploding stars in distant galaxies.
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There are cases in which there are galaxies of counsel and solicitors where it would be unnecessary.
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His calculations suggested that there must be more mass in the universe than those apparent in the observable galaxies, and called this dark matter.
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Small aggregates of galaxies are referred to as groups of galaxies rather than clusters of galaxies.
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From counting dead quasars, he deduced that most massive galaxies have black holes at their centres.
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The infalling material (which contains galaxies, gas and dark matter) gains kinetic energy as it falls into the cluster's gravitational potential well.
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Unfortunately some eleven galaxies had a blue star in the foreground creating the ultraviolet excess, so these galaxies do not really fall into the class.
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Among the objects studied are galaxies, stars, planets, extrasolar planets, the interstellar medium and the cosmic microwave background.
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Imagine looking at two disk galaxies edge-on, one with a bulge and one without a bulge.
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The distribution for lenticular galaxies rises steadily in the range 0.25 to 0.85 whereas the distribution for spirals is essentially flat in that same range.
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Such bars are easy to detect in face-on galaxies, where the structures can be identified visually.
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A group of three foreground galaxies at a redshift of about 1 are behaving as gravitational lenses.
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He has made notable contributions to astronomy in the areas of the evolution of high redshift galaxies, and mass ejection from active galaxies.
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When left alone disks galaxies can rearrange their stars and gas (as a response to instabilities).
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Her work studied the variation in properties of old and new galaxies, including oxygen richness, star formation rate, and the characteristics of the galaxy's nucleus.
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The scope of a science fiction setting is typically larger than that of a fantasy setting, encompassing multiple worlds or even entire galaxies.
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His research interests include observational studies of the formation and evolution of galaxies, clusters of galaxies, and large scale structure in the universe.
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Internal dynamics of stars in galaxies are driven by gravity.
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The absolute magnitudes of galaxies can be much lower (brighter).
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Since the development of the telescope, the field of supernova discovery has expanded to other galaxies.
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As the universe has evolved, galaxies often collide and merge, creating larger galaxies.
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Measuring the aberrations of point-like stars enables corrections to be applied to the images of galaxies during processing.
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As telescopes improved these faint nebulae would be broken into more descriptive scientific classifications such as interstellar clouds, star clusters, and galaxies.
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Blueness in galaxies means that new stars are forming.
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They are thought to form when two galaxies gravitationally interact with each other.
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To take long exposures of galaxies and nebulae, many astronomers use a technique known as auto-guiding.
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At the core, most galaxies have a supermassive black hole, which may result in an active galactic nucleus.
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The cluster consists of two different sub-groups of galaxies with different velocities.
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Between galaxies, there are millions of light-years of this color in the universe.
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The $900,000 computer is being used to simulate supermassive black holes and collisions of galaxies.
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The purpose of the survey is to study the physical processes and evolution of galaxies at redshift z 1.
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Steinmetz is a specialist in the areas of cosmology, the formation and evolution of galaxies and computational astrophysics.
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Recent studies have confirmed the idea that bars are a sign of galaxies reaching full maturity as the formative years end.
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He became a proponent of the so-called island universes hypothesis, which held that spiral nebulae were actually independent galaxies.
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However, its mass is about 27 million solar masses, which means that galaxy's mass to light ratio is around 220.
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He also surveyed the galaxy's stars distribution down to magnitude 19.4.
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An image of an ongoing merger of equal sized disk galaxies is shown left.
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There are also supermassive black holes, which are found at the center of virtually all galaxies.
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A protagonist character disc is placed face down in each of the other galaxies except the home planets of the masters.
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Black hole masses in thousands of galaxies have been estimated in this way.
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A formulation for the number of communicating civilizations in the galaxy.
However, further analysis of wavelengths of the emitted light proved that they were three galaxies merging, and likely two smaller galaxies.
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Other astronomers soon discovered that the void contained a few galaxies.
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They postulated that the rotation of galaxies might be a clue of physical conditions under which these systems formed.
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Subsequent density and pressure fluctuations caused galaxies to form.
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The dust may affect intergalactic distance measurements, such as to supernova and quasars in other galaxies.
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Face-on spiral galaxies have a central 90 km/s; slightly more if viewed edge-on.
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The term commonly refers to the central group of stars found in most spiral galaxies.
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In addition to slowing the overall expansion, gravity causes local clumping of matter into stars and galaxies.
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He claims to be the most intelligent being in at least three galaxies, arguably five.
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The large-scale structure of the universe also looks different if one only uses redshift to measure distances to galaxies.
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In the future, light from distant galaxies will have had more time to travel, so additional regions will become observable.
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If this area is typical for the entire sky, there are over 100 billion galaxies in the universe.
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However, the lensing is strongest in two separated regions near (possibly coincident with) the visible galaxies.
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The quartet is one of the finest examples of compact groups of galaxies.
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Even in our local area of the universe, many galaxies are so dusty that they radiate mainly at those wavelengths.
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The group may contain between 13 and 27 galaxies.
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All the galaxies in these volumes are classified and tallied.
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Applications include simulations of plasmas, galaxies and molecules.
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The galaxies on the list can be observed visually and do not require special photographic or imaging equipment.
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Spiral galaxies have abundant sources for potential star-formation material, but how long galaxies are able to continuously draw on these resources remains in question.
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There are probably more than 170 billion galaxies in the observable universe.
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Collisions occur when two galaxies pass directly through each other and have sufficient relative momentum not to merge.
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Near misses between galaxies result in warping distortions due to tidal interactions, and may cause some exchange of gas and dust.
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Galaxies come in three main types: ellipticals, spirals, and irregulars.
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Were they comming from the centers of distant galaxies?
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The motion of stars in elliptical galaxies is predominantly radial, unlike the disks of spiral galaxies, which are dominated by rotation.
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Stars found inside of elliptical galaxies are very much older than stars found in spiral galaxies.
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He also developed hydrodynamic theory of the spiral structure in galaxies.
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However, not all of these objects are interacting galaxies.
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The distances between galaxies are on the order of a million times further than those between the stars.
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Much closer black hole binaries are likely in single core galaxies with double emission lines.
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Galaxies contain varying numbers of planets, star systems, star clusters and types of interstellar clouds.
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Including galaxies to magnitude 16 would have resulted in an unmanageably large dataset.
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Studies have been also been done of gaseous remnants of exploding stars and the apparently vacant space between members of a cluster of galaxies.
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Spectroscopy is also used to identify the composition of remote objects - like stars and distant galaxies - by analyzing their radiation spectra.
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His primary professional interests lie in cosmology, birth and evolution of galaxies, astronomical instrumentation, and extragalactic astronomy.
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These examples are from corpora and from sources on the web. Any opinions in the examples do not represent the opinion of the Cambridge Dictionary editors or of Cambridge University Press or its licensors.
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