High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Golshan, Roya Hamedani, Sánchez-Monge, Álvaro, Schilke, Peter, Sewiło, Marta, Möller, Thomas, Veena, V. S., Fuller, Gary A.
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Astrophysics of Galaxies
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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