Astrochemistry: September 2019

Scientists supported in part by the NASA Astrobiology Program have developed a new method to analyze mixtures of glycine and glycine oligomers using ion-pair high-performance liquid chromatography (IP-HPLC).

A team of scientists has discovered a new possible pathway toward forming carbon structures in space using a specialized chemical exploration technique at the Department of Energy's Lawrence Berkeley National Laboratory (Berkeley Lab).

We present the observational result of a glycine precursor, methylamine (CH3NH2), together with methanol (CH3OH) and methanimine (CH2NH) towards high-mass star-forming regions, NGC6334I, G10.47+0.03, G31.41+0.3, and W51~e1/e2 using ALMA.