首页> 外文期刊>The Astrophysical journal >CRYSTALLINE SILICATES IN EVOLVED STARS. I. SPITZER/INFRARED SPECTROGRAPH SPECTROSCOPY OF IRAS?16456–3542, 18354–0638, AND 23239+5754
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CRYSTALLINE SILICATES IN EVOLVED STARS. I. SPITZER/INFRARED SPECTROGRAPH SPECTROSCOPY OF IRAS?16456–3542, 18354–0638, AND 23239+5754

机译:演化星中的结晶硅酸盐。 I. IRAS的Spitzer /红外光谱仪?16456–3542、18354-0638和23239 + 5754

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摘要

We report the Spitzer Infrared Spectrograph (IRS) observations of three evolved stars: IRAS?16456–3542, 18354–0638, and 23239+5754. The 9.9-37.2 μm Spitzer/IRS high-resolution spectra of these three sources exhibit rich sets of enstatite-dominated crystalline silicate emission features. IRAS?16456–3542 is extremely rich in crystalline silicates, with 90% of its silicate mass in crystalline form, the highest to date ever reported for crystalline silicate sources.
机译:我们报告了斯必泽红外光谱仪(IRS)对三颗演化恒星的观测:IRAS?16456–3542、18354-0638和23239 + 5754。这三种来源的9.9-37.2μmSpitzer / IRS高分辨率光谱显示出丰富的以顽辉石为主的晶体硅酸盐发射特征集。 IRAS?16456–3542的晶体硅酸盐含量极为丰富,其硅酸盐质量的90%以上为晶体形式,是迄今为止报道的晶体硅酸盐来源中最高的。

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