Becklin–Neugebauer Object
The Becklin–Neugebauer Object (BN) is an object visible only in the infrared in the Orion Molecular Cloud. It was discovered in 1967 by Eric Becklin and Gerry Neugebauer during their near-infrared survey of the Orion Nebula. The BN Object is thought to be an intermediate-mass protostar. It was the first star detected using infrared methods and is deeply embedded within the Orion star-forming nebula, where it is invisible at optical wavelengths because the light is completely scattered or absorbed due to the high density of dusty material.
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Becklin–Neugebauer Object
The Becklin–Neugebauer Object (BN) is an object visible only in the infrared in the Orion Molecular Cloud. It was discovered in 1967 by Eric Becklin and Gerry Neugebauer during their near-infrared survey of the Orion Nebula. The BN Object is thought to be an intermediate-mass protostar. It was the first star detected using infrared methods and is deeply embedded within the Orion star-forming nebula, where it is invisible at optical wavelengths because the light is completely scattered or absorbed due to the high density of dusty material.
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L'objet de Becklin-Neugebauer ...... création de nouvelles étoiles.
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The Becklin–Neugebauer Object ...... igh density of dusty material.
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贝克林-诺伊格鲍尔天体（简称BN天体，英語：Becklin- ...... 5太阳质量。它还是除太阳外在10微米波长以下最为明亮的天体。
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L'objet de Becklin-Neugebauer ...... la dense matière poussiéreuse.
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The Becklin–Neugebauer Object ...... igh density of dusty material.
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贝克林-诺伊格鲍尔天体（简称BN天体，英語：Becklin- ...... 5太阳质量。它还是除太阳外在10微米波长以下最为明亮的天体。
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BN天体
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Becklin–Neugebauer Object
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Objet de Becklin-Neugebauer
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Becklin-Neugebauer Object
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