G327 hot core spectrum analysis

G327.3-0.6 is a very luminous high-mass star-forming hot core at a distance of 3.3 kpc, nearby for a high-mass source. We have obtained ALMA band 6 data at a resolution of 1.9". Then XCLASS software is applied in analyzing the spectra of the hot core. The poster will show the fitted spectra for an example pixel and the physical parameters distribution for the whole hot core.