polar-ring galaxy oor Masedonies
polar-ring galaxy
Vertalings in die woordeboek Engels - Masedonies
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While these galaxies have been extensively studied, many other polar-ring galaxies have since been identified.
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NGC 4650A, an example of a polar-ring galaxy.
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The first four S0 galaxies that were identified as polar-ring galaxies were NGC 2685, NGC 4650A, A 0136 -0801, and ESO 415 -G26.
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One possibility is that a material is tidally stripped from a passing galaxy to produce the polar ring seen in the polar-ring galaxy.
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A polar-ring galaxy is a type of galaxy in which an outer ring of gas and stars rotates over the poles of the galaxy.
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The best-known polar-ring galaxies are S0s (lenticular galaxies), but from the physical point of view they are part of a wider category of galaxies, including several ellipticals.
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In addition to the best-known example, NGC 5128 (Cen A), a very regular polar ring elliptical, is NGC 5266 The SPRC is the Sloan Polar-Ring Catalogue, an atlas of 157 polar-ring galaxies.
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The first polar-ring elliptical galaxies were identified in 1978.
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Polar-ring S0 galaxies may be found around 0.5% of all nearby lenticular galaxies, and it is possible that 5% of lenticular galaxies may have had polar rings at some point during their lifetimes.
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They were NGC 5128, NGC 5363, NGC 1947 and Cygnus A, while the polar-ring S0 galaxies NGC 2685 and NGC 4650A were at that time indicated as resulting from similar formation processes.
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List of galaxies, general list of galaxies Galaxies by type List of spiral galaxies List of ring galaxies List of polar-ring galaxies List of quasars Galaxies by association List of largest known galaxies List of nearest galaxies List of satellite galaxies of the Milky Way Other characterists List of galaxies named after people List of galaxy clusters List of galaxy superclusters List of filaments of galaxies Lists of astronomical objects List of black holes List of clusters List of voids List of the most distant astronomical objects
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These polar rings are thought to form when two galaxies gravitationally interact with each other.
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Only some years later, when the first observations of the stellar and gas motion of polar-ring elliptical and S0 galaxies were possible with a better spectroscopic technology, the external origin of the gaseous rings was clarified.
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The other possibility is that a smaller galaxy collides orthogonally with the plane of rotation of the larger galaxy, with the smaller galaxy effectively forming the polar-ring structure.
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