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The Chemical Classification of the AGB Star IRAS 17515-2407
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作者 Pei-Sheng Chen and Pin Zhang1National Astronomical Observatories, yunnan Observatory, Chinese Academy of Sciences, kunming 650011 2cosmic ray institute, yunnan university, kunming 650091 《Chinese Journal of Astronomy and Astrophysics》 CSCD 北大核心 2003年第6期551-554,共4页
The chemical classification of IRAS 17515-2407 has been debated for a longtime. Up to now there are two contenders, oxygen-rich or carbon-rich. We believe that IRAS17515-2407 is an oxygen-rich source: because (ⅰ) it ... The chemical classification of IRAS 17515-2407 has been debated for a longtime. Up to now there are two contenders, oxygen-rich or carbon-rich. We believe that IRAS17515-2407 is an oxygen-rich source: because (ⅰ) it shows the silicate self-absorbed emission; (ⅱ)in the near infrared-IRAS diagram it is located in the oxygen-rich object region and (ⅲ)particularly, it has detected SiO maser emission. 展开更多
关键词 stars: AGB stars: chemical classification stars: maser infrared: stars
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