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First results of a co survey of the large magellanic cloud with nanten; giant molecular clouds as formation site of populous cluster
(ASTRONOMICAL SOCIETY OF JAPAN, 1999)
First results of a co survey of the large magellanic cloud with nanten; giant molecular clouds as formation site of populous cluster
(ASTRONOMICAL SOCIETY OF JAPAN, 1999)
Molecular clouds and massive star formation in the Magellanic Clouds
(Cappa, C., 2003)
Modelling [CI] emission from turbulent molecular clouds
(Oxford University Press, 2015)
© 2015 The Authors.We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness of the [CI] 609 and 370 μmfine structure emission lines as tracers of cloud structure. Emission from these ...
ALMA Evidence for Ram Pressure Compression and Stripping of Molecular Gas in the Virgo Cluster Galaxy NGC 4402
(IOP Publishing, 2020)
High-resolution (1 '' x 2 '') Atacama Large Millimeter Array CO(2-1) observations of the ram pressure stripped galaxy NGC 4402 in the Virgo cluster show some of the clearest evidence yet for the impacts of ram pressure on ...
The matter between the starsLa materia entre las estrellas
(Facultad de Ciencias, 2010)
LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud
(2010)
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, ...
Fragmentation in filamentary molecular clouds
(OXFORD UNIV PRESS, 2016)
Recent surveys of dust continuum emission at sub-mm wavelengths have shown that filamentary molecular clouds are ubiquitous along the Galactic plane. These structures are inhomogeneous, with overdensities that are sometimes ...
A (C-12)O survey of the Small Magellanic Cloud
(1991-02-10)
The central 2 arcsec x 2 arcsec region of the SMC has been fully surveyed to search for (C-12)O emission in the J = 1-0 transition. (C-12)O emission from two large complexes located in the southwest and northeast regions ...
A complete CO survey of the Large Magellanic Cloud
(1988-08-15)
A complete CO survey of the central 6 deg x 6 deg of the LMC was performed in order to determine the distribution of molecular clouds. At least 10 percent of the region studied exhibits CO line emission, with peak line ...