The structure and dynamics of the 30 Doradus molecular cloud as revealed by ALMA

Autor: Wong, T., Oudshoorn, L., Sofovich, E., Green, A., Indebetouw, R., Meixner, M., Hacar, A., Nayak, O., Tokuda, K., Bolatto, A., Chevance, M., De Marchi, G., Fukui, Y., Hirschauer, A., Jameson, K., Kalari, V., Lebouteiller, V., Looney, L., Madden, S., Onishi, T., Roman-Duval, J., Rubio, M., Tielens, A.G.G.M.

Publikováno v: AAS 240
AAS 240, Jun 2022, Pasadena, United States
Bulletin of the American Astronomical Society, 333.04. AAS
ISSUE=6;STARTPAGE=333.04;TITLE=Bulletin of the American Astronomical Society

International audience; We present results of a wide-field (approximately 60 × 90 pc) ALMA mosaic of CO(2-1) and 13CO(2-1) emission from the molecular cloud associated with the 30 Doradus star-forming region. Three main emission complexes, including

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::07e04e858e681d8735638ab95d432295
https://hal.science/hal-03862727