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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
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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
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.
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