An analysis of water line profiles in star formation regions observed by the Submillimeter Wave Astronomy Satellite
Journal or Book Title
We present spectral line profiles for the 557 GHz 110 → 101 ground-state rotational transition of ortho-H216O for 18 Galactic star formation regions observed by the Submillimeter Wave Astronomy Satellite. Water is unambiguously detected in every source. The line profiles exhibit a wide variety of shapes, including single-peaked spectra and self-reversed profiles. We interpret these profiles using a Monte Carlo code to model the radiative transport. The observed variations in the line profiles can be explained by variations in the relative strengths of the bulk flow and small-scale turbulent motions within the clouds. Bulk flow (infall, outflow) must be present in some cloud cores, and in certain cases this bulk flow dominates the turbulent motions.
Ashby, MLN; Bergin, EA; Plume, R; Carpenter, JM; Neufeld, DA; Chin, G; Erickson, NR; Goldsmith, PF; Harwit, M; Howe, JE; Kleiner, SC; Koch, DG; Patten, BM; Schieder, R; Snell, Ronald L.; Stauffer, JR; Tolls, V; Wang, Z; Winnewisser, G; Zhang, YF; and Melnick, GJ, "An analysis of water line profiles in star formation regions observed by the Submillimeter Wave Astronomy Satellite" (2000). ASTROPHYSICAL JOURNAL. 636.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/636
This document is currently not available here.