The molecular environment of S106 IR

Details The molecular environment of S106 IR The molecular environment of S106 IR

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stin...9419417r&link_type=abstract

Unknown

Astronomy and Astrophysics

Astronomy

Astrography, H Ii Regions, Molecular Clouds, Protostars, Stellar Envelopes, Carbon Compounds, Carbon Monoxide, Cosmic Dust, Data Reduction, Line Spectra, Mapping, Spectrum Analysis

Scientific paper

Millimeter and submillimeter images of the bipolar nebula S106 are presented. The structure of the circumstellar material around the exciting star S106IR is investigated. The previously unresolved 'dust bar' is seen to break up into a number of sources: there is no evidence for a smooth disc about the star. There is a bright, previously undetected far infrared point source in the dust lane which is not detected at 20 micrometers, suggesting it is an extremely embedded object of moderate luminosity which may be a very young protostellar companion to S106 IR.

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