activity
20242026
most citedChemical inventory of the envelope of the Class I protostar L1551 IRS 5

7 citations · 8 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) II. Approach to data reduction and products for line-rich broadband (sub)millimeter spectra

Adele L. Plunkett, Sébastien Maret, Daniel Harsono +26

Studying the chemical composition of the warm gas surrounding embedded solar-type protostars is one of the areas for which the Atacama Large Millimeter/submillimeter Array (ALMA) i…

astro-ph.GA2026

Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS): I. Overview of the ALMA Large Program

J. K. Jørgensen, A. Coutens, M. N. Drozdovskaya +27

It remains a fundamental research question in astrochemistry to characterize the inventory of complex organic molecules formed during the early stages of star formation, which may…

astro-ph.GA2026

Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) III. CHOH isotopic fractionation in the low-mass protostar BHR71-IRS1

A. Coutens, F. Cruz-Sáenz de Miera, J. K. Jørgensen +26

[Abridged] Methanol is a complex organic molecule detected in both ice and gas toward star-forming regions. Due to its high abundance, its rarer isotopologues, including the deuter…

astro-ph.SR2026

Chemical Complexity in the Early Stages of Star Formation in the SKAO Era

Eleonora Bianchi, Mathilde Bouvier, Claudio Codella +44

About 350 molecules have been identified in the interstellar medium (ISM), including complex molecules relevant to prebiotic chemistry. A remarkable level of molecular diversity ha…

astro-ph.GA2025

The evolution of complex organic molecules during star formation

Pierre Marchand, Audrey Coutens, Jean-Christophe Loison +3

Complex organic molecules (COMs) are thought to be the precursors of pre-biotic molecules and are observed in many protostellar sources. For this paper we studied the formation of…

astro-ph.SR2025

APE: An analytical protostellar environment to provide physical conditions to chemical models and synthetic observations

Pierre Marchand, Audrey Coutens, Antoine Espagnet +3

Chemical modeling and synthetic observations are powerful methods to interpret observations, both requiring a knowledge of the physical conditions. In this paper, we present the An…

astro-ph.GA2024★ 7 cited

Chemical inventory of the envelope of the Class I protostar L1551 IRS 5

P. Marchand, A. Coutens, J. Scigliuto +5

Episodic accretion in protostars leads to luminosity outbursts that end up heating their surroundings. This rise in temperature pushes the snow lines back, enabling the desorption…

astro-ph.EP2024★ 1 cited

Protoplanetary disk size under non-ideal magnetohydrodynamics: A general formalism with inclined magnetic field

Yueh-Ning Lee, Barshan Ray, Pierre Marchand +1

Many mechanisms have been proposed to alleviate the magnetic catastrophe, which prevents the Keplerian disk from forming inside a collapsing magnetized core. Such propositions incl…