Herschel observations of Extra-Ordinary Sources: H2S as a Probe of Dense Gas and Possibly Hidden Luminosity Toward the Orion KL Hot Core
arXiv:1401.2470 · doi:10.1088/0004-637X/781/2/114
Abstract
We present Herschel/HIFI observations of the light hydride HS obtained from the full spectral scan of the Orion Kleinmann-Low nebula (Orion KL) taken as part of the HEXOS GT key program. In total, we observe 52, 24, and 8 unblended or slightly blended features from HS, HS, and HS, respectively. We only analyze emission from the so called hot core, but emission from the plateau, extended ridge, and/or compact ridge are also detected. Rotation diagrams for ortho and para HS follow straight lines given the uncertainties and yield T=14112 K. This indicates HS is in LTE and is well characterized by a single kinetic temperature or an intense far-IR radiation field is redistributing the population to produce the observed trend. We argue the latter scenario is more probable and find that the most highly excited states (E>1000 K) are likely populated primarily by radiation pumping. We derive an HS column density, N(HS)=9.51.910 cm, gas kinetic temperature, T=120 K, and constrain the H volume density, n>910 cm, for the HS emitting gas. These results point to an HS origin in markedly dense, heavily embedded gas, possibly in close proximity to a hidden self-luminous source (or sources), which are conceivably responsible for Orion KL's high luminosity. We also derive an HS ortho/para ratio of 1.70.8 and set an upper limit for HDS/H2S of <4.910.
46 pages, 13 figures, 6 tables. Accepted for publication to ApJ
References in corpus (5)
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