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A portrait of cold gas in galaxies at 60 pc resolution and a simple method to test hypotheses that link small-scale ism structure to galaxy-scale processes
(IOP Publishing, 2016)
The cloud-scale density, velocity dispersion, and gravitational boundedness of the interstellar medium (ISM) vary within and among galaxies. In turbulent models, these properties play key roles in the ability of gas to ...
IRAS 16547−4247: a new candidate of a protocluster unveiled with ALMA
(The American Astronomical Society, 2015-01-10)
We present the results of continuum and 12CO(3–2) and CH3OH(7–6) line observations of IRAS 16547−4247
made with the Atacama Large Millimeter/submillimeter Array (ALMA) at an angular resolution of ∼0.
5. The
12CO(3–2) ...
IRAS 16547−4247: A New Candidate of a Protocluster Unveiled with ALMA
(American Astronomical Society, 2015)
We present the results of continuum and 12CO(3–2) and CH3OH(7–6) line observations of IRAS 16547−4247
made with the Atacama Large Millimeter/submillimeter Array (ALMA) at an angular resolution of ∼0.
5. The
12CO(3–2) ...
A two-component power law covering nearly four orders of magnitude in the power spectrum of spitzer far-infrared emission from the large magellanic cloud
(The Astrophysical Journal Letters, 2010)
ISM properties in hydrodynamic galaxy simulations: Turbulence cascades, cloud formation, role of gravity and Feedback
(Monthly Notices of the Royal Astronomical Society, 2010)