N-bearing complex organics toward high-mass protostars: constant ratios pointing to formation in similar pre-stellar conditions across a large mass range

Author(s):
Nazari, P. (0000-0002-4448-3871); Meijerhof, J.D.; Gelder, M.L. van (0000-0002-6312-8525); Ahmadi, M.; Dishoeck, E.F. van (0000-0001-7591-1907); Tabone, B.; Langeroodi, D.; Ligterink, N.F.W.; Jaspers, J.; Beltrán, M.T.; Fuller, G.A.; Sánchez-Monge, Á.; Schilke, P.
Published
2022
Publication type
Article / Letter to editor
AstrochemistryStarsMassive starsProtostarsISM AbundancesTechniquesInterferometricStars pre-main sequenceAstrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A109
hdl
1887/3513593
doi
10.1051/0004-6361/202243788
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...668A.109N