Infrared Low-Resolution Spectra of HAEBE Stars

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Chen P S Wang X H He J H Yunnan Observatory and United Laboratory for Optical Astronomy The Chinese Academy of SciencesKunming China National Astronomical Observatories CAS China [650011 ]
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IRAS low-resolution spectra are presented for 36 HAEBE stars. It is found that silicate dust in amorphous or glassy form is common material in the circumstellar disks or/and shells of HAEBE stars. It is also found that the PAH feature is often appeared as well.
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