Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-06-20
Astrophys.J.646:L57-L60,2006
Astronomy and Astrophysics
Astrophysics
4 pages, color, to appear in ApJL
Scientific paper
10.1086/507026
A recent submillimeter line survey of Orion KL claimed detection of SiH. This paper reports on GBT observations of the 5.7 GHz Lambda-doubling transitions of SiH in Orion. Many recombination lines, including C164-delta, are seen, but SiH is not detected. The nondetection corresponds to an upper limit of 1.5 x 10^15 cm^-2 (4 sigma) for the beam-averaged column density of SiH. This suggests that the fractional abundance of SiH in the extended ridge is no more than twice that in the hot core.
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