Far-infrared detection of a circumstellar dust torus around Sharpless 106

Details Far-infrared detection of a circumstellar dust torus around Sharpless 106 Far-infrared detection of a circumstellar dust torus around Sharpless 106

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...316l..75h&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 316, May 15, 1987, p. L75-L80.

Astronomy and Astrophysics

Astrophysics

9

Angular Resolution, Cosmic Dust, Far Infrared Radiation, Infrared Detectors, Stellar Coronas, Stellar Envelopes, Bipolarity, Maximum Entropy Method, Molecular Gases

Scientific paper

High angular resolution scans at 42 and 95 μm have been obtained of the far-infrared source associated with S106. Using maximum entropy deconvolution techniques the authors find that the far-IR-emitting dust appears to be distributed in a toroidal shape around the central star. This result is similar to the morphology implied by millimeter line and continuum mapping on a variety of size scales.

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