4 papers
Accurate laboratory rest frequencies of vibrationally excited CO up to and up to 2 THz
R. Gendriesch, F. Lewen, G. Klapper +4
Astronomical observations of (sub)millimeter wavelength pure rotational emission lines of the second most abundant molecule in the Universe, CO, hold the promise of probing regions…
Extended [C I] and ^{13}CO(5-4) Emission in M17SW
J. E. Howe, M. L. N. Ashby, E. A. Bergin +19
We mapped a 13 by 22 pc region in emission from 492 GHz [C I] and, for the first time, 551 GHz ^{13}CO(5-4) in the giant molecular cloud M17SW, using the Submillimeter Wave Astrono…
The Distribution of Water Emission in M17SW
R. L. Snell, J. E. Howe, M. L. N. Ashby +17
We present a 17-point map of the M17SW cloud core in the 1_{10}-1_{01} transition of ortho-water at 557 GHz obtained with the Submillimeter Wave Astronomy Satellite. Water emission…
Atomic Carbon in M82: Physical conditions derived from simultaneous observations of the [CI] fine structure submillimeter wave transitions
J. Stutzki, U. U. Graf, S. Haas +10
We report the first extragalactic detection of the neutral carbon [CI] 3P2-3P1 fine structure line at 809 GHz. The line was observed towards M82 simultaneously with the 3P1-3P0 lin…