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Time evolution of o-H$_2$D$^+$, N$_2$D$^+$, and N$_2$H$^+$ during the high-mass star formation process

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Sabatini, G., Bovino, S., Redaelli, E., Wyrowski, F., Urquhart, J. S., Giannetti, A., Brand, J., Menten, K. M.
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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