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(1 - 4 of 4)
The 30 doradus molecular cloud at 0.4 pc resolution with the atacama large millimeter/submillimeter array
Wong, T.; Oudshoorn, L.; Sofovich, E.; Green, A.; Shah, C.; Indebetouw, R.; ... ; Tielens, A.G.G.M. 2022
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
Article / Letter to editor
open access
First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C II]-bright Gas and CO-bright Gas at Low Metallicity
Jameson, K.E.; Bolatto, A.D.; Wolfire, M.; Warren, S.R.; Herrera-Camus, R.; Croxall, K.; ... ; Okada, Y. 2018
First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C II]-bright Gas and CO-bright Gas at Low Metallicity
Article / Letter to editor
open access
Dust Emission at 8 and 24 μm as Diagnostics of H II Region Radiative Transfer
Oey, M.S.; López-Hernández, J.; Kellar, J.A.; Pellegrini, E.W.; Gordon, K.D.; Jameson, K.E.; ... ; Tielens, A.G.G.M. 2017
Dust Emission at 8 and 24 μm as Diagnostics of H II Region Radiative Transfer
Article / Letter to editor
open access
The Relationship Between Molecular Gas, H I, and Star Formation in the Low-mass, Low-metallicity Magellanic Clouds
Jameson, K.E.; Bolatto, A.D.; Leroy, A.K.; Meixner, M.; Roman-Duval, J.; Gordon, K.; ... ; Sonneborn, G. 2016
The Relationship Between Molecular Gas, H I, and Star Formation in the Low-mass, Low-metallicity Magellanic Clouds
Article / Letter to editor
open access