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The Effects of Grain Size and Temperature Distributions on the Formation of Interstellar Ice Mantles
Tyler Pauly, Robin T. Garrod
Computational models of interstellar gas-grain chemistry have historically adopted a single dust-grain size of 0.1 micron, assumed to be representative of the size distribution pre…
Exploring molecular complexity with ALMA (EMoCA): Alkanethiols and alkanols in Sagittarius B2(N2)
H. S. P. Müller, A. Belloche, L. -H. Xu +7
Over the past five decades, radio astronomy has shown that molecular complexity is a natural outcome of interstellar chemistry, in particular in star forming regions. However, the…
Exploring Molecular Complexity with ALMA (EMoCA): Deuterated complex organic molecules in Sagittarius B2(N2)
A. Belloche, H. S. P. Müller, R. T. Garrod +1
Deuteration is a powerful tracer of the history of the cold prestellar phase in star forming regions. Apart from methanol, little is known about deuterium fractionation of complex…
Formation of hydroxylamine on dust grains via ammonia oxidation
Jiao He, Gianfranco Vidali, Jean-Louis Lemaire +1
The quest to detect prebiotic molecules in space, notably amino acids, requires an understanding of the chemistry involving nitrogen atoms. Hydroxylamine (NHOH) is considered a…
Complex organic molecules in organic-poor massive young stellar objects
Edith C. Fayolle, Karin I. Öberg, Robin T. Garrod +2
Massive young stellar objects (MYSOs) with hot cores are classic sources of complex organic molecules. The origins of these molecules in such sources, as well as the small- and lar…