Приклади вживання Elliptical galaxies Англійська мовою та їх переклад на Українською
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They are called elliptical galaxies.
Elliptical galaxies, as the name implies, are elliptical in shape.
They are not seen in elliptical galaxies.
Massive elliptical galaxies have high Sérsic indices and a high degree of central concentration.
These galaxies are called elliptical galaxies.
Elliptical galaxies are divided into three'stages': compact ellipticals(cE), normal ellipticals(E) and late types(E+).
At the centre of the cluster are several massive elliptical galaxies.
It was thought that massive elliptical galaxies formed as a result of collisions of galactic disks.
These systems alsohave abundant interstellar gas(unlike other Elliptical galaxies).
The outcome is that in elliptical galaxies, only about 40 percent of the available gas fell into that central region.
Other regions that did not happen to pick up a rotationwould become oval objects called elliptical galaxies.
Magneto-hydrodynamic processes in active elliptical galaxies produce their characteristic jets and radio lobes.
Other regions, which did not happen to pick up a rotation,would become oval-shaped objects called elliptical galaxies.
In this study, researchers show that in elliptical galaxies only 40 percent of free gas falls to the central region.
Previous studies of distant dead galaxies haveassumed that their structure is similar to the local elliptical galaxies they will evolve into.
Although the largest elliptical galaxies formed all or most of their stars more than 10 billion years ago, super spirals are still forming stars today.
These winds are also presumed to be responsible for the existence of“red and dead” elliptical galaxies, in which no new stars can form.
Tyson describes how elliptical galaxies, in which some of the oldest red dwarf stars exist, would offer the best chance of finding established civilizations.
These winds are also believed to be responsible for the presence of“red and dead” elliptical galaxies, in which no new stars can develop.
Unlike most elliptical galaxies, however, Centaurus A's smooth shape is disturbed by a broad and patchy band of dark material that obscures the galaxy's centre.
Over billions of years,this merging process assembled the large spiral and elliptical galaxies that now appear to be common in the modern Universe.
In giant elliptical galaxies, most measurements come from observations of the orbital motion of stars around the black hole, taken in visible or infrared light.
Because they lack stellar nurseries andcontain mostly old stars, elliptical galaxies are often considered“dead” when compared to their spiral relatives.
For instance, galaxies have been discovered that, in a certain sense,occupy an intermediate position between spiral and elliptical galaxies(identified as SO).
However, unlike Mrk 1216, most giant elliptical galaxies continued to gradually grow in size when smaller galaxies merged with them over cosmic time….
Tens of percents of ULXs are in fact background quasars; the probability for a ULX tobe a background source is larger in elliptical galaxies than in spiral galaxies. .
In giant elliptical galaxies, a number of measurements arise from observations of the orbital motion of stars around the black hole, taken in infrared or visible light.
In previous studies, it was assumed that distant deadgalaxies were similar in structure to the local elliptical galaxies they eventually evolved into.
Approximately 75% of LINER galaxies are either elliptical galaxies, lenticular galaxies, or S0/a-Sab galaxies(spiral galaxies with large bulges and tightly wound spiral arms).
Tens of percents of ULXs are in fact background quasars; the probability for a ULX tobe a background source is larger in elliptical galaxies than in spiral galaxies. .