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The molecular ridge close to 30 doradus in the large magellanic cloud
Jürgen Ott
,
Tony Wong
, Jorge L. Pineda
, Annie Hughes
, Erik Muller
, Zhi Yun Li
, Min Wang
, Lister Staveley-Smith
, Yasuo Fukui
, Axel Weiß
, Christian Henkel
, Ulrich Klein
Astronomy
Research output
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peer-review
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Keyphrases
Interferometric
100%
Large Magellanic Cloud
100%
Molecular Gas
100%
Overdensity
100%
HCO+
100%
Australia
50%
High Density
50%
Shear Force
50%
Molecular Complexes
50%
Opacity
50%
Structure Transition
50%
Pressure Force
50%
Ar Pressure
50%
Velocity Components
50%
Emission Peak
50%
Star Formation
50%
Massive Stars
50%
High Opacity
50%
Single Disc
50%
Shell-like Structures
50%
Velocity Structure
50%
Compact Array
50%
Tidal Force
50%
Gas Tracer
50%
Molecular Cloud Formation
50%
Shock Force
50%
Formation History
50%
Earth and Planetary Sciences
Magellanic Clouds
100%
Molecular Gas
100%
Emissions
50%
Australia
50%
Molecular Clouds
50%
Massive Star
50%
Star Formation
50%
Velocity Structure
50%
Gas Density
50%
Physics
Large Magellanic Cloud
100%
Molecular Gas
100%
Star Formation
50%
Molecular Clouds
50%
Massive Star
50%