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Cited article:

ALMA resolves molecular clouds in metal-poor Magellanic Bridge A

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THE 1.1 mm CONTINUUM SURVEY OF THE SMALL MAGELLANIC CLOUD: PHYSICAL PROPERTIES AND EVOLUTION OF THE DUST-SELECTED CLOUDS*

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K-band integral field spectroscopy and optical spectroscopy of massive young stellar objects in the Small Magellanic Cloud

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Interpreting the sub-linear Kennicutt–Schmidt relationship: the case for diffuse molecular gas

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Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC

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On the relationship between molecular hydrogen and carbon monoxide abundances in molecular clouds

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Modelling CO emission - I. CO as a column density tracer and the X factor in molecular clouds

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THE CO-TO-H2CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUP

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The Astrophysical Journal 737 (1) 12 (2011)
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LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud

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THE INFLUENCE OF FAR-ULTRAVIOLET RADIATION ON THE PROPERTIES OF MOLECULAR CLOUDS IN THE 30 DOR REGION OF THE LARGE MAGELLANIC CLOUD

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CONSTRAINING THE STAR FORMATION HISTORIES OF GAMMA-RAY BURST HOST GALAXIES FROM THEIR OBSERVED ABUNDANCE PATTERNS

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The state of molecular gas in the Small Magellanic Cloud

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Tracing the cold molecular gas reservoir through dust emission in the SMC

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The Resolved Properties of Extragalactic Giant Molecular Clouds

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CO and CS in the Magellanic Clouds: a $\mathsf{\chi^2}$-analysis of multitransitional data based on the MEP radiative transfer model

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TheSpitzerSurvey of the Small Magellanic Cloud: Far‐Infrared Emission and Cold Gas in the Small Magellanic Cloud

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Millimeter dust continuum emission revealing the true mass of giant molecular clouds in the Small Magellanic Cloud

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[CII] 158 μm emission and metallicity in photon dominated regions

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HST/ACS observations of the old and metal-poor Sagittarius dwarf irregular galaxy

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High Excitation Molecular Gas in the Magellanic Clouds

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