The Infrared Variation of the Symbiotic Star BI Cru

Details The Infrared Variation of the Symbiotic Star BI Cru The Infrared Variation of the Symbiotic Star BI Cru

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..359n&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

We have obtained observations of six symbiotic stars with Spitzer MIPS
(photometery at 24 μm and 70 μm) and IRS (spectroscopic range
9.9-37.2 μm). Here we report the presence of 10 μm and 18
μm dust features in one of these stars, BI Cru, which were not
observed in ISO spectra of the same system.

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