The ALMA-PILS survey: First detections of ethylene oxide, acetone and propanal toward the low-mass protostar IRAS 16293-2422
A&A, 597 (2017) A53
Published online: 2016-12-21
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Astrochemical evolution along star formation: overview of the IRAM Large Program ASAI
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Exploring the Origins of Earth’s Nitrogen: Astronomical Observations of Nitrogen-bearing Organics in Protostellar Environments
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The ALMA-PILS survey: Stringent limits on small amines and nitrogen-oxides towards IRAS 16293–2422B
N. F. W. Ligterink, H. Calcutt, A. Coutens, et al.Astronomy & Astrophysics 619 A28 (2018)
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First detection of cyanamide (NH2CN) towards solar-type protostars
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The ALMA-PILS survey: isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293–2422B
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The ALMA-PILS survey: the sulphur connection between protostars and comets: IRAS 16293–2422 B and 67P/Churyumov–Gerasimenko
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Tracing the cold and warm physico-chemical structure of deeply embedded protostars: IRAS 16293−2422 vs. VLA 1623−2417
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Complex organic molecules in the Galactic Centre: the N-bearing family
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The ALMA-PILS Survey: Formaldehyde deuteration in warm gas on small scales toward IRAS 16293–2422 B
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First hot corino detected around an isolated intermediate-mass protostar: Cep E-mm
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Tunnelling dominates the reactions of hydrogen atoms with unsaturated alcohols and aldehydes in the dense medium
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The formation of peptide-like molecules on interstellar dust grains
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The ALMA-PILS survey: first detection of methyl isocyanide (CH3NC) in a solar-type protostar
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Detection of methyl isocyanate (CH3NCO) in a solar-type protostar
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On the Formation of the C2H6O Isomers Ethanol (C2H5OH) and Dimethyl Ether (CH3OCH3) in Star-forming Regions
Alexandre Bergantini, Pavlo Maksyutenko and Ralf I. KaiserThe Astrophysical Journal 841 (2) 96 (2017)
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Observation and Analysis of Interstellar Acetone in GAL 31.41+0.31, GAL 034.3+00.2, and GAL 10.47+00.03
Luyao Zou and Susanna L. Widicus WeaverThe Astrophysical Journal 849 (2) 139 (2017)
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The ALMA-PILS survey: detection of CH3NCO towards the low-mass protostar IRAS 16293−2422 and laboratory constraints on its formation
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