SAO 206462 - a solar-type star with a dusty, organically rich environment

Details SAO 206462 - a solar-type star with a dusty, organically rich environment SAO 206462 - a solar-type star with a dusty, organically rich environment

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.274..977c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 4, pp. 977-986.

Astronomy and Astrophysics

Astronomy

27

Polarization, Circumstellar Matter, Stars: Individual: Sao 206462, Dust, Extinction, Infrared: Stars

Scientific paper

We report photometric, polarimetric and spectroscopic observations of SAO 206462 in the optical, near-infrared and submillimetre. The system has near- and far-infrared excesses, and emissions from atomic hydrogen and PAH molecules. We interpret these data and the IRAS far-infrared photometry in terms of a dusty environment around the star. SAO 206462 is unique in being a solar-type, Vega-excess star with an organic component to its surrounding dust.

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