activity
20142025
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 · 2.4k across the 34 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2023★ 3 cited

Protostellar Interferometric Line Survey of the Cygnus-X region (PILS-Cygnus) -- The role of the external environment in setting the chemistry of protostars

S. J. van der Walt, L. E. Kristensen, H. Calcutt +2

(Abridged) Molecular lines are commonly detected towards protostellar sources. However, to get a better understanding of the chemistry of these sources we need unbiased molecular s…

astro-ph.GA2023★ 8 cited

Episodic infall towards a compact disk in B335?

Per Bjerkeli, Jon P. Ramsey, Daniel Harsono +7

Previous observations of B335 have presented evidence of ongoing infall in various molecular lines, e.g., HCO, HCN, CO. There have been no confirmed observations of a rotationa…

astro-ph.GA2022

The prebiotic molecular inventory of Serpens SMM1: II. The building blocks of peptide chains

Niels F. W. Ligterink, Aida Ahmadi, Bijaya. Luitel +7

This work aims to constrain the abundances of interstellar amides, by searching for this group of prebiotic molecules in the intermediate-mass protostar Serpens SMM1-a. ALMA observ…

astro-ph.GA2019★ 34 cited

The ALMA-PILS survey: Gas dynamics in IRAS 162932422 and the connection between its two protostars

M. H. D. van der Wiel, S. K. Jacobsen, J. K. Jørgensen +10

[Abridged] The majority of stars form in binary or higher order systems. The Class 0 protostellar system IRAS16293-2422 contains two protostars, 'A' and 'B', separated by ~600 au a…

astro-ph.GA2018★ 42 cited

The ALMA-PILS survey: first detection of methyl isocyanide (CHNC) in a solar-type protostar

H. Calcutt, M. R. Fiechter, E. R. Willis +9

Methyl isocyanide (CHNC) is the isocyanide with the largest number of atoms confirmed in the interstellar medium (ISM), but it is not an abundant molecule, having only been det…

astro-ph.GA2018★ 115 cited

The ALMA-PILS survey: Complex nitriles towards IRAS 16293--2422

H. Calcutt, J. K. Jørgensen, H. S. P. Müller +8

Complex organic molecules are readily detected in the inner regions of the gaseous envelopes of forming protostars. In particular, molecules that contain nitrogen are interesting d…

astro-ph.GA2017★ 72 cited

The ALMA-PILS survey: Formaldehyde deuteration in warm gas on small scales toward IRAS 16293-2422 B

M. V. Persson, J. K. Jørgensen, H. S. P. Müller +7

[abridged] The enhanced degrees of deuterium fractionation observed in envelopes around protostars demonstrate the importance of chemistry at low temperatures, relevant in pre- and…

astro-ph.GA2014★ 75 cited

Laboratory Characterization and Astrophysical Detection of Vibrationally Excited States of Vinyl Cyanide in Orion-KL

A. López, B. Tercero, Z. Kisiel +11

New laboratory data of CHCHCN (vinyl cyanide) in its ground and vibrationally excited states at the microwave to THz domain allow searching for these excited state transitions…