ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars. Motivation, sample, calibration, and initial results

ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars. Motivation, sample, calibration, and initial resultsDOI: info:10.1051/0004-6361/202140431v. 660A94
Gottlieb, C. A., Decin, L., Richards, A. M. S., De Ceuster, F., Homan, W., Wallström, S. H. J., Danilovich, T., Millar, T. J., Montargès, M., Wong, K. T., McDonald, I., Baudry, A., Bolte, J., Cannon, E., De Beck, E., de Koter, A., El Mellah, I., Etoka, S., Gobrecht, D., Gray, M., Herpin, F., Jeste, M., Kervella, P., Khouri, T., Lagadec, E. et al. 2022. "ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars. Motivation, sample, calibration, and initial results." Astronomy and Astrophysics, 660 A94. https://doi.org/10.1051/0004-6361/202140431.
ID: 167243
Type: article
Keywords: SAO