High-Resolution X-ray Observations of the Orion Nebula

作者: W. H.-M. KU , G. RIGHINI-COHEN , M. SIMON

DOI: 10.1126/SCIENCE.215.4528.61

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摘要: Observations of the Trapezium region in Orion Nebula obtained with high-resolution x-ray imaging instrument on board Einstein Observatory reveal at least 58 sources emission. All but two can be identified visible stars. The strongest source is star Θ 1 C, which excites emission nebula. Its luminosity 6 x 10 32 ergs per second. rest may stars all spectral types. Strong not observed from members infrared cluster embedded within molecular cloud .

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