Приклади вживання Spiral arms Англійська мовою та їх переклад на Українською
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They are usually found in the spiral arms of galaxies.
The stars in its spiral arms orbit around its center about once every several hundred million years.
They possess both a bulge and a disk, but lack spiral arms.
Scientists measured magnetic fields along the spiral arms of the galaxy called NGC 1068, or M77.
The Meathook Galaxy, or NGC 2442, in the southern constellation of Volans(The Flying Fish),is easily recognised for its asymmetric spiral arms.
Scientists measured magnetic fields along the spiral arms of the galaxy called NGC 1068, or Messier 77.
The spiral arms of the galaxy M106 bright stretched at this wonderful heavenly portrait-mosaic, composed of ground-based and space-based images.
I have used the most common names for the spiral arms on this map.
About half a dozen prominent spiral arms can be seen, each containing large amounts of gas and dust.
Through our simulations we have shown for the first time that even if you change gravity,it would not prevent disc galaxies with spiral arms from forming.".
The bluish feature in the spiral arms indicate the presence of young stars born out of clouds of interstellar gas.
For the study, scientists measured magnetic fields along the spiral arms of the galaxy called NGC 1068, or M77.
The Milky Way has multiple spiral arms, long curved streams of gas and stars stretching out from the galactic centre.
Active star formation takes place in the disk(especially in the spiral arms, which represent areas of high density).
In the picture you can see spiral arms of the galaxy, lit by the diffuse glow of thousands of stars as well as strands of dark cosmic dust.
Active star formation takes place in the disk(especially in the spiral arms, which represent areas of high density).
It was found that the galaxy which spiral arms are twisted anticlockwise, there is 7% more than the galaxies with“opposite orientation”.
Outside the gravitational influence of the Galactic bar, the structure of the interstellar medium andstars in the disk of the Milky Way is organized into four spiral arms.
They are usually observed in the spiral arms of galaxies and in H II regions, but not in elliptical galaxies.
Gravitational interactions between galaxies in the group have also left telltale signs,including the warped and inflated disk of NGC 3628 and the drawn out spiral arms of M66.
Type II supernovae are mainly observed in the spiral arms of galaxies and in H II regions, but not in elliptical galaxies.
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).
The only place where the speeds of stars and spiral arms coincide- the so-called corotational circle, and it is the Sun.
This flurry of activity is shown by theunmistakable blue-hued knots speckling the galaxy's spiral arms, each of which marks a clump of hot newborn stars.
One interesting feature of this galaxy is that its spiral arms wind all the way into the center, so that ESO 498-G5's core looks like a bit like a miniature spiral galaxy.
The most distinctive features of the bright galaxy NGC 3521 are its long spiral arms that are dotted with star-forming regions and interspersed with veins of dust.
Such pairs are thought necessary to draw out the spiral arms in which new stars and their associated planetary systems are preferentially formed.
Flocculent spirals-- galaxies without well defined spiral arms-- are a quite common form of galaxy, and NGC 4414 is one of the closest.