Inventories of Rich Carbon-Chain Chemistry in Prestellar and Starless Cores in the Perseus Molecular Cloud
National Radio Astronomy Observatory · National Radio Astronomy Observatory · RIKEN Cluster for Pioneering Research · Steward Observatory, University of Arizona · Centro de Astrobiología · Centro de Astrobiología
astro-ph.GA, astro-ph.EP, astro-ph.SR
Submitted: 2026-08-05
Updated: 2026-09-18
Comments: Accepted for publication in MNRAS. 21-page main text (with 12 figures) and 19-page appendix (with 2 figures) for a total of 40 pages
Code: https://github.com/andresmegias/gildas-class-pipeline
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation
- From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation
- Deuterium Fractionation: the Ariadne's Thread from the Pre-collapse Phase to Meteorites and Comets today
- Organic chemistry in the first phases of Solar-type protostars
- c-C3H2 deuteration towards prestellar and starless cores in the Perseus Molecular Cloud
- Array Programming with NumPy
- From Bubbles and Filaments to Cores and Disks: Gas Gathering and Growth of Structure Leading to the Formation of Stellar Systems
- An Observational Perspective of Low-Mass Dense Cores I: Internal Physical and Chemical Properties
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