Anatomy of the Class I protostar L1489 IRS with NOEMA

Context. Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions are associated with the emission of particular molecular lines, allowing us to use molecular probes of the YSO...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2024-07, Vol.687
Hauptverfasser:	Tanious, M, R. Le Gal, Neri, R, Faure, A, Gupta, A, Law, C J, Huang, J, Cuello, N, Williams, J P, Ménard, F
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrochemistry Binary stars Bubbles Data analysis Emission analysis External pressure Line spectra Molecular gases Outflow Spatial distribution Spectral resolution
Online-Zugang:	Volltext
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