306 citations · 3.8k across the 52 of their papers we have counts for
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The ALMA-PILS survey: The first detection of doubly-deuterated methyl formate (CHD2OCHO) in the ISM
S. Manigand, H. Calcutt, J. K. Jørgensen +9
Studies of deuterated isotopologues of complex organic molecules can provide important constraints on their origin in regions of star formation. In particular, the abundances of de…
The census of interstellar complex organic molecules in the Class I hot corino of SVS13-A
E. Bianchi, C. Codella, C. Ceccarelli +12
We present the first census of the interstellar Complex Organic Molecules (iCOMs) in the low-mass Class I protostar SVS13-A, obtained by analysing data from the IRAM-30m Large Proj…
Can Formamide Be Formed on Interstellar Ice? An Atomistic Perspective
Albert Rimola, Dimitrios Skouteris, Nadia Balucani +4
Interstellar formamide (NH2CHO) has recently attracted significant attention due to its potential role as a molecular building block in the formation of precursor biomolecules rele…
The ALMA-PILS survey: Isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293-2422B
J. K. Jørgensen, H. S. P. Müller, H. Calcutt +7
This paper presents a systematic survey of the deuterated and 13C isotopologues of a variety of oxygen-bearing complex organic molecules on Solar System scales toward the protostar…
The formation of peptide-like molecules on interstellar dust grains
N. F. W. Ligterink, J. Terwisscha van Scheltinga, V. Taquet +4
Molecules with an amide functional group resemble peptide bonds, the molecular bridges that connect amino acids, and may thus be relevant in processes that lead to the formation of…
First Detection of the Simplest Organic Acid in a Protoplanetary Disk
Cécile Favre, Davide Fedele, Dmitry Semenov +14
The formation of asteroids, comets and planets occurs in the interior of protoplanetary disks during the early phase of star formation. Consequently, the chemical composition of th…
Linking interstellar and cometary O: a deep search for OO in the solar-type protostar IRAS 16293--2422
Vianney Taquet, Ewine F. van Dishoeck, Matthew Swayne +15
Recent measurements carried out at comet 67P/C-G with the probe revealed that molecular oxygen, O, is the fourth most abundant molecule in comets. Models show t…
Low levels of methanol deuteration in the high-mass star-forming region NGC 6334I
Eva G. Bøgelund, Brett A. McGuire, Niels F. W. Ligterink +6
The abundance of deuterated molecules in a star-forming region is sensitive to the environment in which they are formed. Deuteration fractions therefore provide a powerful tool for…
The evolution of grain mantles and silicate dust growth at high redshift
Cecilia Ceccarelli, Serena Viti, Nadia Balucani +1
In dense molecular clouds, interstellar grains are covered by mantles of iced molecules. The formation of the grain mantles has two important consequences: it removes species from…
Seeds of Life in Space (SOLIS). III. Zooming into the methanol peak of the pre-stellar core L1544
Anna Punanova, Paola Caselli, Siyi Feng +41
Towards the pre-stellar core L1544, the methanol (CHOH) emission forms an asymmetric ring around the core centre, where CHOH is mostly in solid form, with a clear peak 4000…
Imaging the water snowline in a protostellar envelope with HCO
Merel L. R. van 't Hoff, Magnus V. Persson, Daniel Harsono +5
Snowlines are key ingredients for planet formation. Providing observational constraints on the locations of the major snowlines is therefore crucial for fully connecting planet com…