ALMA Observations of the Spatial Distribution of three C$_2$H$_4$O$_2$ Isomers towards Sgr B2(N)
Ci Xue (1), Anthony J. Remijan (2), Andrew M. Burkhardt (1), Eric, Herbst (1) ((1) University of Virginia, (2) National Radio Astronomy, Observatory)

TL;DR
This study uses ALMA interferometric observations to analyze the spatial distribution and velocity components of three C$_2$H$_4$O$_2$ isomers in Sgr B2(N), revealing distinct morphologies and chemical process implications.
Contribution
It introduces a quantitative selection method for uncontaminated transitions and reports new detections, providing detailed spatial and velocity analysis of the isomers.
Findings
HCOOCH$_3$ and CH$_2$OHCHO each show two velocity components.
HCOOCH$_3$ distribution is extended and offset from continuum.
CH$_2$OHCHO and CH$_3$COOH have similar, compact distributions.
Abstract
The CHO isomers have been previously investigated primarily via disparate sets of observations involving single dish and array measurements. The only attempt at using a uniform set of observations was performed with the IRAM 30 m observation in 2013 (Belloche et al. 2013). In this study, we present an intensive and rigorous spectral and morphological analysis of the CHO isomers towards Sgr B2(N) with interferometers, ALMA Band 3 observations. We propose a quantitative selection method, which automates the determination of the most uncontaminated transitions and allows us to report the discovery of previously undetected transitions of the three isomers. With the least contaminated transitions, the high spatial-resolution millimeter maps of the CHO isomers reveal that HCOOCH and CHOHCHO each display two different velocity components, while only…
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