A Study of Multiple Molecular Lines at the 3 mm Band toward Gas Infalling Sources

Abstract The study of multiple molecular spectral lines in gas infalling sources can provide the physical and chemical properties of these sources and help us estimate their evolutionary stages. We report line detections within the 3 mm band using the FTS wide-sideband mode of the IRAM 30 m telescope toward 20 gas-infalling sources. Using XCLASS, we identify the emission lines of up to 22 molecular species (including a few isotopologues) and one hydrogen radio recombination line in these sources. H 13 CO + , HCO + , HCN, HNC, c-C 3 H 2 , and CCH lines are detected in 15 sources. We estimate the rotation temperatures and column densities of these molecular species using the LTE radiative transfer model, and compare the molecular abundances of these sources with those from nine high-mass star-forming regions reported in previous studies and with those from the chemical model. Our results suggest that G012.79-0.20, G012.87-0.22 clump A and B, and G012.96-0.23 clump A may be in the high-mass protostellar object stage, while sources with fewer detected species may be in the earlier evolutionary stage. Additionally, the CCH and c-C 3 H 2 column densities in our sources reveal a linear correlation, with a ratio of N (CCH)/ N (c-C 3 H 2 ) = 89.2 ± 5.6, which is higher than the ratios reported in the literature. When considering only sources with lower column densities, this ratio decreases to 29.0 ± 6.1, consistent with those of diffuse clouds. Furthermore, a comparison between the N (CCH)/ N (c-C 3 H 2 ) ratio and the sources’ physical parameters reveals a correlation, with sources exhibiting higher ratios tending to have higher kinetic temperatures and H 2 column densities.