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The relationship between CO emission and visual extinction traced by dust emission in the Magellanic Clouds
Cheoljong Lee, Adam K. Leroy, Scott Schnee, et al. Monthly Notices of the Royal Astronomical Society 450(3) 2708 (2015) https://doi.org/10.1093/mnras/stv863
ASTE observations in the 345 GHz window towards the HII region N113 of the Large Magellanic Cloud
13CO(J = 1–0) On-the-Fly Mapping of the Giant H II Region NGC 604: Variation in Molecular Gas Density and Temperature due to Sequential Star Formation
Kazuyuki Muraoka, Tomoka Tosaki, Rie Miura, Sachiko Onodera, Nario Kuno, Kouichiro Nakanishi, Hiroyuki Kaneko and Shinya Komugi Publications of the Astronomical Society of Japan 64(1) (2012) https://doi.org/10.1093/pasj/64.1.3
Physical properties of giant molecular clouds in the Large Magellanic Cloud
Submillimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined fromJ = 3–2 andJ = 1–0 Transitions of CO
Tetsuhiro Minamidani, Norikazu Mizuno, Yoji Mizuno, et al. The Astrophysical Journal Supplement Series 175(2) 485 (2008) https://doi.org/10.1086/524038
High Excitation Molecular Gas in the Magellanic Clouds
Alberto D. Bolatto, Frank P. Israel and Christopher L. Martin The Astrophysical Journal 633(1) 210 (2005) https://doi.org/10.1086/432928
Tiny-scale molecular structures in the Magellanic Clouds