ALMA reveals molecular cloud N55 in the Large Magellanic Cloud as a site of massive star formation. (2018)
Keywords :
galaxies ISM; ISM: molecules; Magellanic Clouds; stars: formation stars: massive; stars: protostars
Abstract:We present the molecular cloud properties of N55 in the Large Magellanic Cloud using ^12^CO(1-0) and ^13^CO(1-0) observations obtained with Atacama Large Millimeter Array. We have done a detailed study of molecular gas properties, to understand how the cloud properties of N55 differ from Galactic clouds. Most CO emission appears clumpy in N55, and molecular cores that have young stellar objects (YSOs) show larger linewidths and masses. The massive clumps are associated with high and intermediate mass YSOs. The clump masses are determined by local thermodynamic equilibrium and virial analysis of the ^12^CO and ^13^CO emissions. These mass estimates lead to the conclusion that (a) the clumps are in self-gravitational virial
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N55 was observed with ALMA in cycle 1 and 2 (2013.1.00214.S and
2012.1.00335.S), using band 3 receivers in spectral windows centered
at 115.27, 110.20, and 109.67GHz, with 70.557kHz (0.2km/s) spectral
resolution.
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