The 30 doradus molecular cloud at 0.4 pc resolution with the atacama large millimeter/submillimeter array: physical properties and the boundedness of CO-emitting structures

Author(s):
Wong, T.; Oudshoorn, L.; Sofovich, E.; Green, A.; Shah, C.; Indebetouw, R.; Meixner, M.; Hacar, A.; Nayak, O.; Tokuda, K.; Bolatto, A.D.; Chevance, M.; De Marchi, G.; Fukui, Y.; Hirschauer, A.S.; Jameson, K.E.; Kalari, V.; Lebouteiller, V.; Looney, L.W.; Madden, S.C.; Onishi, T.; Roman-Duval, J.; Rubio, M.; Tielens, A.G.G.M.
Published
2022
Publication type
Article / Letter to editor
Interstellar mediumMagellanic cloudsMillimeter astronomyGiant molecular cloudsStar forming regions84799010616531565Astrophysics - astrophysics of galaxies
Date issued
2022
Language
English
Is part of
The Astrophysical Journal (2022), No. 1, 47
hdl
1887/3562550
doi
10.3847/1538-4357/ac723a
URL
https://ui.adsabs.harvard.edu/abs/2022ApJ...932...47W