The Chemical Classification of the AGB Star IRAS 17515--2407

Details The Chemical Classification of the AGB Star IRAS 17515--2407 The Chemical Classification of the AGB Star IRAS 17515--2407

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjaa...3..551c&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, No. 6, p. 551-554

Astronomy and Astrophysics

Astrophysics

Stars: Agb, Stars: Chemical Classification, Stars: Maser Infrared: Stars

Scientific paper

The chemical classification of IRAS 17515--2407 has been debated for a long time. Up to now there are two contenders, oxygen-rich or carbon-rich. We believe that IRAS 17515--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.

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