LWS observations of the bright rimmed globule IC 1396N.

Details LWS observations of the bright rimmed globule IC 1396N. LWS observations of the bright rimmed globule IC 1396N.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...315l.293s&link_type=abstract

Astronomy and Astrophysics, v.315, p.L293-L296

Astronomy and Astrophysics

Astrophysics

39

Stars: Formation, Ism: Jets And Outflows, Ism: Individual Objects: Ic 1396N, Infrared: Ism:Lines

Scientific paper

We present the first far-infrared spectrum of the IRAS source associated with IC 1396N, located in the HII region IC 1396 together with submillimeter and millimeter photometry. A rich spectrum of CO, OH, and H_2_O lines are detected in the ISO-LWS spectrum, indicative of a warm, dense region, probably shock excited, around the source. Among the fine structure lines, [OIII] and [NIII] are also detected and can be explained by the presence of the O6 star HD206267 approximately 16pc away. The far infrared and submillimeter spectral energy distribution is fitted with a model assuming spherical grey-bodies with a radial power law of density and temperature. An accurate measure of the bolometric luminosity and an estimate of the total envelope mass are obtained.

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