Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution: insights from the IRAM NOEMA large programme CORE

Author(s):
Ahmadi, A. (0000-0003-4037-5248); Beuther, H.; Bosco, F.; Gieser, C.; Suri, S.; Mottram, J.C.; Kuiper, R.; Henning, T.; Sánchez-Monge, Á.; Linz, H.; Pudritz, R.E.; Semenov, D.; Winters, J.M.; Möller, T.; Beltrán, M.T.; Csengeri, T.; Galván-Madrid, R.; Johnston, K.G.; Keto, E.; Klaassen, P.D.; Leurini, S.; Longmore, S.N.; Lumsden, S.L.; Maud, L.T.; Moscadelli, L.; Palau, A.; Peters, T.; Ragan, S.E.; Urquhart, J.S.; Zhang, Q.; Zinnecker, H.
Published
2023
Publication type
Article / Letter to editor
Stars: formationStars: massiveStars: kinematics and dynamicsTechniques: interferometricAstrophysics - Astrophysics of GalaxiesAstrophysics - Solar and Stellar Astrophysics
Date issued
2023
Language
English
Is part of
Astronomy and Astrophysics (2023), A171
hdl
1887/3717206
doi
10.1051/0004-6361/202245580
URL
https://ui.adsabs.harvard.edu/abs/2023A&A...677A.171A