Mapping of the Orion molecular cloud in the [CII] line and continuum at 158 μm

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

A fabry Perot Spectrometer (FPS) tuned to the astrophysically interesting (CII) line at 157.7409 ?m, developed at ISAS (Japan) has been successfully interfaced to the TIFR 100 cm far-infrared balloon borne telescope. A region (30? x 15?) of the Orion molecular cloud was mapped with a spectral resolution of 1700 and angular resolution of ~ 1?. The spatial distribution of (CII) line emission at 157.7409 ?m and the neighboring dust continuum are presented here.

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