作者: Harold M. Butner , Helen J. Walker , Diane H. Wooden , Fred C. Witteborn
DOI: 10.1017/S0252921100014664
关键词: Main sequence 、 Comet 、 Astronomy 、 Interplanetary dust cloud 、 Spectral line 、 Cosmic dust 、 Physics 、 Stars 、 Astronomical spectroscopy 、 Infrared excess 、 Astrophysics
摘要: Beta Pic is a nearby main-sequence star with an extended dust disk, large infrared excess, and mid-infrared emission similar to that seen in some cometary spectra. We selected sample of stars whose properties resemble obtained 8 13 micron spectra (resolution 200). find variety silicate features among the our sample, ranging from classic interstellar comet P/Halley laboratory Interplanetary Dust Particles (IDP's).