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The 13CO(2–1)/12CO(2–1) Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud

  • Authors: Dia Kalra, Erik Rosolowsky, Adam Leroy, Remy Indebetouw

Dia Kalra et al 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

Caption: Figure 1.

(left) Herschel SPIRE 500 μm dust continuum map of the LMC displayed on a logarithmic stretch. Circles indicate the positions of the ALMA fields. (right) Correlation between 12CO and 13CO for 100 GMCs in the LMC. The points are color-coded by the far-infrared luminosity ﹩(\mathrm{log}{L}_{\,\rm{FIR}\,})﹩ from YSOs inside the molecular clouds. The red dashed line represents the ensemble mean ratio (R13 = 0.082).

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)

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