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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Bibliographic Details
Main Authors:	Sabatini, G., Bovino, S., Redaelli, E., Wyrowski, F., Urquhart, J. S., Giannetti, A., Brand, J., Menten, K. M.
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2411.14530