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radioastronómico - translation to English
radioastronomy
![opacity]]) of various [[wavelength]]s of electromagnetic radiation.](https://commons.wikimedia.org/wiki/Special:FilePath/Atmospheric electromagnetic opacity.svg?width=200 "opacity]]) of various [[wavelength]]s of electromagnetic radiation.")
![Chart on which [[Jocelyn Bell Burnell]] first recognised evidence of a [[pulsar]], in 1967 (exhibited at [[Cambridge University Library]])](https://commons.wikimedia.org/wiki/Special:FilePath/Chart Showing Radio Signal of First Identified Pulsar.jpg?width=200 "Chart on which [[Jocelyn Bell Burnell]] first recognised evidence of a [[pulsar]], in 1967 (exhibited at [[Cambridge University Library]])")
![A radio image of the central region of the Milky Way galaxy. The arrow indicates a supernova remnant which is the location of a newly discovered transient, bursting low-frequency radio source [[GCRT J1745-3009]].](https://commons.wikimedia.org/wiki/Special:FilePath/GCRT J1745-3009 2.jpg?width=200 "A radio image of the central region of the Milky Way galaxy. The arrow indicates a supernova remnant which is the location of a newly discovered transient, bursting low-frequency radio source [[GCRT J1745-3009]].")
![Antenna 70 m of the [[Goldstone Deep Space Communications Complex]], [[California]]](https://commons.wikimedia.org/wiki/Special:FilePath/Goldstone DSN antenna.jpg?width=200 "Antenna 70 m of the [[Goldstone Deep Space Communications Complex]], [[California]]")
![Green Bank radio telescope]], USA](https://commons.wikimedia.org/wiki/Special:FilePath/Green Bank Telescope.jpg?width=200 "Green Bank radio telescope]], USA")
![[[Grote Reber]]'s Antenna at [[Wheaton, Illinois]], world's first parabolic radio telescope](https://commons.wikimedia.org/wiki/Special:FilePath/Grote Antenna Wheaton.gif?width=200 "[[Grote Reber]]'s Antenna at [[Wheaton, Illinois]], world's first parabolic radio telescope")
![HST]]), a radio image of same galaxy using '''Interferometry''' ([[Very Large Array]] – '''VLA'''), and an image of the center section ('''VLBA''') using a ''Very Long Baseline Array'' (Global VLBI) consisting of antennas in the US, Germany, Italy, Finland, Sweden and Spain. The jet of particles is suspected to be powered by a [[black hole]] in the center of the galaxy.](https://commons.wikimedia.org/wiki/Special:FilePath/M87 VLA VLBA radio astronomy.jpg?width=200 "HST]]), a radio image of same galaxy using '''Interferometry''' ([[Very Large Array]] – '''VLA'''), and an image of the center section ('''VLBA''') using a ''Very Long Baseline Array'' (Global VLBI) consisting of antennas in the US, Germany, Italy, Finland, Sweden and Spain. The jet of particles is suspected to be powered by a [[black hole]] in the center of the galaxy.")
![The [[Atacama Large Millimeter Array]] (ALMA), many antennas linked together in a radio interferometer](https://commons.wikimedia.org/wiki/Special:FilePath/The Atacama Compact Array.jpg?width=200 "The [[Atacama Large Millimeter Array]] (ALMA), many antennas linked together in a radio interferometer")
SUBFIELD OF ASTRONOMY THAT STUDIES CELESTIAL OBJECTS AT RADIO FREQUENCIES
Radioastronomy; Radio Astronomy; Radio and Radar Astronomy; Radio astronomer; Radio Astronomer; Millimeter-wave astronomy; Radio astronomy service; Radio astronomy station; Microwave astronomy; History of radio astronomy; Radio astronomers
radioastronómico [Noun]
radioastronómico
radio-astronomical
