Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)
Arnaud Belloche, Holger S. P. M\"uller, Karl M. Menten, Peter Schilke,, Claudia Comito

TL;DR
This study conducted an extensive spectral line survey of Sagittarius B2(N) and (M) using the IRAM 30m telescope, revealing a high level of chemical complexity and identifying numerous molecules, including several detected in space for the first time.
Contribution
It provides the most comprehensive spectral line survey of Sgr B2 to date, identifying new molecules and excited states, and advancing understanding of interstellar organic chemistry.
Findings
Detected about 3675 and 945 spectral lines toward N and M.
Identified 56 and 46 molecules, including new space detections.
Discovered aminoacetonitrile, n-propyl cyanide, and ethyl formate in space.
Abstract
The discovery of amino acids in meteorites and the detection of glycine in samples returned from a comet to Earth suggest that the interstellar chemistry is capable of producing such complex organic molecules. Our goal is to investigate the degree of chemical complexity that can be reached in the ISM. We performed an unbiased, spectral line survey toward Sgr B2(N) and (M) with the IRAM 30m telescope in the 3mm window. The spectra were analyzed with a simple radiative transfer model that assumes LTE but takes optical depth effects into account. About 3675 and 945 spectral lines with a peak signal-to-noise ratio higher than 4 are detected toward N and M, i.e. about 102 and 26 lines per GHz, respectively. This represents an increase by about a factor of 2 over previous surveys of Sgr B2. About 70% and 47% of the lines detected toward N and M are identified and assigned to 56 and 46…
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