Traducción y análisis de palabras por inteligencia artificial ChatGPT
En esta página puede obtener un análisis detallado de una palabra o frase, producido utilizando la mejor tecnología de inteligencia artificial hasta la fecha:
- cómo se usa la palabra
- frecuencia de uso
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- etimología
radio galaxy - traducción al ruso
![3C31]]. Jets and plumes are labelled.](https://commons.wikimedia.org/wiki/Special:FilePath/Radio galaxy 3C31.png?width=200 "3C31]]. Jets and plumes are labelled.")
![[[Pseudo-colour]] image of the large-scale radio structure of the FRII radio galaxy 3C98. Lobes, jet and hotspot are labelled.](https://commons.wikimedia.org/wiki/Special:FilePath/Radio galaxy 3C98.png?width=200 "[[Pseudo-colour]] image of the large-scale radio structure of the FRII radio galaxy 3C98. Lobes, jet and hotspot are labelled.")
[reidiəu'gæləksi]
астрономия
радиогалактика
![[[NGC 1300]] in [[infrared]] light.](https://commons.wikimedia.org/wiki/Special:FilePath/HAWK-I NGC 1300.jpg?width=200 "[[NGC 1300]] in [[infrared]] light.")
![Tuning-fork-style diagram of the [[Hubble sequence]]](https://commons.wikimedia.org/wiki/Special:FilePath/HubbleTuningFork.jpg?width=200 "Tuning-fork-style diagram of the [[Hubble sequence]]")
![Spiral galaxy [[NGC 1345]]](https://commons.wikimedia.org/wiki/Special:FilePath/NGC 1345 HST.jpg?width=200 "Spiral galaxy [[NGC 1345]]")
![The bright galaxy [[NGC 3810]] demonstrates classical spiral structure in this very detailed image from Hubble. Credit: ESA/Hubble and NASA.](https://commons.wikimedia.org/wiki/Special:FilePath/NGC 3810 (captured by the Hubble Space Telescope).jpg?width=200 "The bright galaxy [[NGC 3810]] demonstrates classical spiral structure in this very detailed image from Hubble. Credit: ESA/Hubble and NASA.")
![Spiral galaxy [[NGC 6384]] taken by [[Hubble Space Telescope]].](https://commons.wikimedia.org/wiki/Special:FilePath/NGC 6384 HST.jpg?width=200 "Spiral galaxy [[NGC 6384]] taken by [[Hubble Space Telescope]].")
![WISE]] data](https://commons.wikimedia.org/wiki/Special:FilePath/PIA19341-MilkyWayGalaxy-SpiralArmsData-WISE-20150603.jpg?width=200 "WISE]] data")
![[[Barred spiral galaxy]] [[UGC 12158]].](https://commons.wikimedia.org/wiki/Special:FilePath/UGC 12158.jpg?width=200 "[[Barred spiral galaxy]] [[UGC 12158]].")
![[[Frequency]] spectrum of a typical modulated AM or FM radio signal. It consists of a component ''C'' at the [[carrier wave]] frequency <math>f_c</math> with the information ([[modulation]]) contained in two narrow bands of frequencies called [[sideband]]s (''SB'') just above and below the carrier frequency.](https://commons.wikimedia.org/wiki/Special:FilePath/Modulated radio signal frequency spectrum.svg?width=200 "[[Frequency]] spectrum of a typical modulated AM or FM radio signal. It consists of a component ''C'' at the [[carrier wave]] frequency <math>f_c</math> with the information ([[modulation]]) contained in two narrow bands of frequencies called [[sideband]]s (''SB'') just above and below the carrier frequency.")
![Radio communication. Information such as sound is converted by a transducer such as a [[microphone]] to an electrical signal, which modulates a [[radio wave]] produced by the [[transmitter]]. A receiver intercepts the radio wave and extracts the information-bearing modulation signal, which is converted back to a human usable form with another transducer such as a [[loudspeaker]].](https://commons.wikimedia.org/wiki/Special:FilePath/Signal processing system.png?width=200 "Radio communication. Information such as sound is converted by a transducer such as a [[microphone]] to an electrical signal, which modulates a [[radio wave]] produced by the [[transmitter]]. A receiver intercepts the radio wave and extracts the information-bearing modulation signal, which is converted back to a human usable form with another transducer such as a [[loudspeaker]].")
![Volkswagen's RNS-510 receiver supports [[Sirius Satellite Radio]].](https://commons.wikimedia.org/wiki/Special:FilePath/SiriusXM Display on Volkswagen's RNS-510 Receiver.png?width=200 "Volkswagen's RNS-510 receiver supports [[Sirius Satellite Radio]].")
![shows its own photo]]](https://commons.wikimedia.org/wiki/Special:FilePath/Wireless network.jpg?width=200 "shows its own photo]]")
радиотехника
радиопередача
Definición
Wikipedia
A radio galaxy is a galaxy with giant regions of radio emission extending well beyond its visible structure. These energetic radio lobes are powered by jets from its active galactic nucleus. They have luminosities up to 1039 W at radio wavelengths between 10 MHz and 100 GHz. The radio emission is due to the synchrotron process. The observed structure in radio emission is determined by the interaction between twin jets and the external medium, modified by the effects of relativistic beaming. The host galaxies are almost exclusively large elliptical galaxies. Radio-loud active galaxies can be detected at large distances, making them valuable tools for observational cosmology. Recently, much work has been done on the effects of these objects on the intergalactic medium, particularly in galaxy groups and clusters.
Alcyoneus is a low-excitation radio galaxy, identified as having the largest radio lobes found, with lobed structures spanning 5 megaparsecs (16×106 ly). For comparison, another similarly sized giant radio galaxy is 3C 236, with lobes 15 million light-years across. A giant radio galaxy is a special class of objects characterized by the presence of radio lobes generated by relativistic jets powered by the central galaxy's supermassive black hole. Giant radio galaxies are different from ordinary radio galaxies in that they can extend to much larger scales, reaching upwards to several megaparsecs across, far larger than the diameters of their host galaxies.
