activity
20122022
most citedThe ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA

402 citations · 1.3k across the 11 of their papers we have counts for

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Showing 2016 · astro-ph.SRShow all

5 papers · 2 filters

astro-ph.SR2016

The ALMA-PILS survey: First detections of ethylene oxide, acetone and propanal toward the low-mass protostar IRAS 16293-2422

J. M. Lykke, A. Coutens, J. K. Jørgensen +14

One of the open questions in astrochemistry is how complex organic and prebiotic molecules are formed. Aims. Our aim is to start the process of compiling an inventory of oxygen-bea…

astro-ph.SR2016★ 30 cited

Water around IRAS15398-3359 observed with ALMA

P. Bjerkeli, J. K. Jørgensen, E. A. Bergin +9

How protostars accrete mass is one of the fundamental problems of star formation. High column densities and complex kinematical structures make direct observations challenging and…

astro-ph.SR2016★ 402 cited

The ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA

J. K. Jørgensen, M. H. D. van der Wiel, A. Coutens +14

The inner regions of the envelopes surrounding young protostars are characterised by a complex chemistry, with prebiotic molecules present on the scales where protoplanetary disks…

astro-ph.SR2016

The ALMA-PILS survey: First detections of deuterated formamide and deuterated isocyanic acid in the interstellar medium

A. Coutens, J. K. Jørgensen, M. H. D. van der Wiel +15

Formamide (NHCHO) has previously been detected in several star-forming regions and is thought to be a precursor for different prebiotic molecules. Its formation mechanism is st…

astro-ph.SR2016

Constraining the physical structure of the inner few 100 AU scales of deeply embedded low-mass protostars

M. V. Persson, D. Harsono, J. J. Tobin +4

(Abridged) The physical structure of deeply-embedded low-mass protostars (Class 0) on scales of less than 300 AU is still poorly constrained. Determining this is crucial for unders…