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Synthetic
26
Al emission from galactic-scale superbubble simulations
D. Rodgers-Lee
,
M. G. H. Krause
, J. Dale
, R. Diehl
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
:
Contribution to journal
›
Article
›
peer-review
18
Citations (Scopus)
36
Downloads (Pure)
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26
Al emission from galactic-scale superbubble simulations'. Together they form a unique fingerprint.
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Keyphrases
Galactic
100%
26Al
100%
Superbubbles
100%
Galaxies
50%
Milky Way
30%
Spiral Arms
20%
Line-of-sight Velocity
20%
Measurement Location
10%
All-sky
10%
Gas Density
10%
Halo
10%
3D Hydrodynamics
10%
Radioactive Decay
10%
High Integrated
10%
Morphological Characteristics
10%
Cold Gas
10%
Massive Stars
10%
Trace Elements
10%
High Velocity
10%
Systematic Variation
10%
Doppler Shift
10%
Gamma-ray Emission
10%
Star Formation Rate
10%
High Latitude
10%
Hydrodynamic Simulation
10%
Gray Intensity
10%
Velocity Diagram
10%
Emission Map
10%
Time Location
10%
Scale Height
10%
Galactic Rotation
10%
Physics
Superbubbles
100%
Milky Way
60%
Line of Sight
40%
Spiral Arms
40%
Gamma Radiation
40%
Scale Height
20%
Cold Gas
20%
Star Formation Rate
20%
Massive Star
20%
Galactic Rotation
20%
Radioactive Decay
20%
Doppler Effect
20%