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The big ears of radio astronomy

Bibliographic Data

ID12416822
AuthorsF G Smith (0000-0001-6436-256X, SKA Observatory, corresponding author), Francis Graham-Smith
Year2002
Volume10
Issue2
Pages285-300
Publication date2002-05-01
Open AccessYes
TypeARTICLE
VenueEuropean Review (JOURNAL)
Journal identifiersISSN: 1062-7987 • E-ISSN: 1474-0575
PublisherCambridge University Press (CUP) (PUBLISHER)
DOI10.1017/s1062798702000200
OpenAlexW2012029604
LanguageEN

The special value of radio astronomy lies in the probing of extreme conditions in the universe, including the highest energies and the lowest temperatures. Radio waves can penetrate clouds of gas and dust to reveal objects in the universe and, in particular, in our Galaxy that cannot be seen by visible light. To achieve the highest resolution, radio telescopes in widely separate parts of our globe combine their reception to produce a synthesized image. This is a splendid example of international collaboration. Among the images visualized are pulsars, derived from the remnants of supernovae explosions, and quasar sources powered by black holes

Astronomy · Astrophysics · Galaxy · Physics · Pulsar · Quasar · Radio astronomy · Radio galaxy · Radio telescope · Radio wave · Supernova · Universe · History and Developments in Astronomy · Radio Astronomy Observations and Technology

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