CHEMICAL DIAGNOSTICS OF THE MASSIVE STAR CLUSTER-FORMING CLOUD G33.92+0.11. I. 13CS, CH3OH, CH3N, OCS, H2S, SO2, and SiO
Authors: Young Chol Minh, Hauyu Baobab Liu, and Roberto Galvań-Madrid
2016 The Astrophysical Journal82499.
Provider: AAS Journals
Caption: Figure 7.
Sample spectra taken toward the positions A and B in Figure 6(a). The red lines show the Gaussian fit results for the narrow component. The integrated intensity of this narrow component is shown as the gray background of Figure 6(a).
