Far-Infrared CO Rotational Lines in the Orion Molecular Cloud

Details Far-Infrared CO Rotational Lines in the Orion Molecular Cloud Far-Infrared CO Rotational Lines in the Orion Molecular Cloud

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..205s&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 205-208 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a high signal-to-noise grating spectrum between 43-196.9
μm of the Orion molecular cloud towards the massive star-forming
region IRc2, obtained with the Long Wavelength Spectrometer (LWS) on
board the Infrared Space Observatory (ISO).

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