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

Wong, T.; Oudshoorn, L.; Sofovich, E.; Green, A.; Shah, C.; Indebetouw, R.; ... ; Tielens, A.G.G.M. (2022)

Article / Letter to editor

• Interstellar medium
• Magellanic clouds
• Millimeter astronomy
• Giant molecular clouds
• Star forming regions
• 847
• 990
• 1061
• 653
• 1565
• Astrophysics - astrophysics of galaxies

• All authors: 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.
• Date: 2022
• Journal: The Astrophysical Journal
• Volume: 932
• Issue: 1
• DOI: doi:10.3847/1538-4357/ac723a
• Link: https://ui.adsabs.harvard.edu/abs/2022ApJ...932...47W