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CHEMICAL DIVERSITY IN HIGH-MASS STAR FORMATION
2008
Astronomical Journal
Massive star formation exhibits an extremely rich chemistry. However, not much evolutionary details are known yet, especially at high spatial resolution. Therefore, we synthesize previously published Submillimeter Array high-spatial-resolution spectral line observations toward four regions of high-mass star formation that are in various evolutionary stages with a range of luminosities. Estimating column densities and comparing the spatially resolved molecular emission allows us to characterize
doi:10.1088/0004-6256/137/1/406
fatcat:lle3ndm7dnavdfsyfua37j4bw4