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- W4308243334 abstract "The studies of the complex molecular lines towards the hot molecular cores at millimeter and submillimeter wavelengths provide instructive knowledge about the chemical complexity in the interstellar medium (ISM). We presented the detection of the rotational emission lines of the complex nitrogen-bearing molecule ethyl cyanide (C$_{2}$H$_{5}$CN) towards the hot molecular core G10.47+0.03 using the Atacama Large Millimeter/Submillimeter Array (ALMA) band 4 observations. The estimated column density of C$_{2}$H$_{5}$CN towards the G10.47+0.03 was 7.7($pm$0.5)$times$10$^{16}$ cm$^{-2}$ with the high rotational temperature of 352.9$pm$66.8 K. The estimated fractional abundance of C$_{2}$H$_{5}$CN with respect to H$_{2}$ towards the G10.47+0.03 was 5.70$times$10$^{-9}$. We observed that the estimated fractional abundance of C$_{2}$H$_{5}$CN is similar to the simulated abundance of C$_{2}$H$_{5}$CN which was predicted by the three-phase warm-up model from Garrod (2013). We also discuss the possible formation mechanism of C$_{2}$H$_{5}$CN towards the hot molecular cores and we claim the barrierless and exothermic radical-radical reaction between CH$_{2}$ and CH$_{2}$CN is responsible for the production of low abundant C$_{2}$H$_{5}$CN ($sim$10$^{-9}$) in the grain surface of the G10.47+0.03." @default.
- W4308243334 created "2022-11-09" @default.
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- W4308243334 date "2022-11-03" @default.
- W4308243334 modified "2023-09-25" @default.
- W4308243334 title "Detection of complex nitrogen-bearing molecule ethyl cyanide towards the hot molecular core G10.47+0.03" @default.
- W4308243334 doi "https://doi.org/10.48550/arxiv.2211.01608" @default.
- W4308243334 hasPublicationYear "2022" @default.
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