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IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

Fuente: arXiv

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Bibliographic Details
Main Authors:	Watson, Dan M., Narang, Mayank, Pittman, Caeley V., Tyagi, Himanshu, Gutermuth, Robert, Rubinstein, Adam E., Evans II, Neal J., Hartmann, Lee W., Megeath, S. Thomas, Manoj, P., Espaillat, Catherine C., Calvet, Nuria, Garatti, Alessio Caratti o, van Dishoeck, Ewine F., Bourke, Tyler L., Green, Joel D., Lisse, Carey M., Klaassen, Pamela, Looney, Leslie W., Nazari, Pooneh, Neufeld, David A., Tobin, John J., Wolk, Scott J., Anglada, Guillem, Atnagulov, Prabhani, Beuther, Henrik, Brunken, Nashanty G. C., Federman, Samuel, Furlan, Elise, Habel, Nolan, Karnath, Nicole, Linz, Hendrik, Page, James Muzerolle, Osorio, Mayra, Pokhrel, Riwaj, Rahatgaonkar, Rohan, Rocha, Will R. M., Sheehan, Patrick D., Slavicinska, Katerina, Stanke, Thomas, Stutz, Amelia M., Tychoniec, Lukasz, Yang, Yao-Lun, Fischer, William J.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2512.15999