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- W3100806568 abstract "Context. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, at low metallicities especially, CO only traces the shielded interiors of the clouds. In this context, millimeter dust emission can be used as a tracer to unveil the total dense gas masses. However, the comparison of masses deduced from the continuum SIMBA 1.2 mm emission and virial masses (understood to trace the entire potential of the clouds) in a sample of giant molecular clouds in the Small Magellanic Cloud (SMC) by previous studies found a discrepancy between these two quantities that requires explanation." @default.
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- W3100806568 date "2010-11-23" @default.
- W3100806568 modified "2023-10-02" @default.
- W3100806568 title "LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud" @default.
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- W3100806568 doi "https://doi.org/10.1051/0004-6361/200913372" @default.
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