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单词 Becklin–Neugebauer Object
释义
Becklin–Neugebauer Object

Astronomy
  • A powerful source of infrared radiation discovered by the American astronomers Eric Edward Becklin (1940– ) and Gerry (born Gerhart Otto) Neugebauer (1932–2014) in 1966 behind the Orion Nebula; the dense gas and dust of the Orion Nebula completely obscures it from optical telescopes. It is thought to be either a massive and highly luminous protostar, or a runaway star ejected from the Trapezium region of the Orion Nebula.


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