Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Magnus V. Persson"'
Autor:
John J. Tobin, Merel L. R. van ’t Hoff, Margot Leemker, Ewine F. van Dishoeck, Teresa Paneque-Carreño, Kenji Furuya, Daniel Harsono, Magnus V. Persson, L. Ilsedore Cleeves, Patrick D. Sheehan, Lucas Cieza
Publikováno v:
Nature. 615:227-230
Autor:
Yoshihide Yamato, Kenji Furuya, Yuri Aikawa, Magnus V. Persson, John J. Tobin, Jes K. Jørgensen, Mihkel Kama
Publikováno v:
Yamato, Y, Furuya, K, Aikawa, Y, Persson, M V, Tobin, J J, Jorgensen, J K & Kama, M 2022, ' The First Interferometric Measurements of NH 2 D/NH 3 Ratio in Hot Corinos ', Astrophysical Journal, vol. 941, no. 1, 75 . https://doi.org/10.3847/1538-4357/ac9ea5
The nitrogen chemical evolution during star and planet formation is still not fully understood. Ammonia (NH$_3$) is a key specie in the understanding of the molecular evolution in star-forming clouds and nitrogen isotope fractionation. In this paper,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be4c1d6a08e28eabc201715af629c33d
http://arxiv.org/abs/2210.16336
http://arxiv.org/abs/2210.16336
Autor:
Adam Ginsburg, Brigitta M. Sipőcz, C. E. Brasseur, Philip S. Cowperthwaite, Matthew W. Craig, Christoph Deil, James Guillochon, Giannina Guzman, Simon Liedtke, Pey Lian Lim, Kelly E. Lockhart, Michael Mommert, Brett M. Morris, Henrik Norman, Madhura Parikh, Magnus V. Persson, Thomas P. Robitaille, Juan-Carlos Segovia, Leo P. Singer, Erik J. Tollerud
Publikováno v:
Astronomical Journal; Mar2019, Vol. 157 Issue 3, p1-1, 1p