ISO observations of XX Oph

Details ISO observations of XX Oph ISO observations of XX Oph

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..305e&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 305

Physics

Xx Oph, Model Atmospheres, Uir Emission

Scientific paper

We present ISO SWS and PHOT-P observations of the binary XX Oph. The UIR features seen in ground-based data are confirmed. The near infrared is modelled by a 3400 K log g=3.5 giant, which is likely to be underabundant in carbon. There is an infrared excess at long wavelengths, corresponding to emission by dust having temperature 336 K and β-index 0.4.

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