The internal kinematics of the Large Magellanic Cloud (LMC) disk have been modeled by several studies using different tracers with varying coverage, resulting in a range of parameters. Here, we model the LMC disk using 1705 star clusters and field stars,
S. R. Dhanush+2 more
doaj +1 more source
Studies of the Large Magellanic Cloud. V. The Young Populous Clusters.
P. W. Hodge
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The Radio Continuum of the Large Magellanic Cloud. III. The Sources at 11 cm Wavelength [PDF]
R. X. McGee, JW Brooks, R. Batchelor
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Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
Search for 8-80 KEV X-Rays from the Large Magellanic Cloud and the Crab Nebula
F. D. Seward, A. Toor
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On the Structure of the Magnetic Field in the Large Magellanic Cloud [PDF]
J. Isserstedt, Michael Reinhardt
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High-precision density mapping of marine debris and floating plastics via satellite imagery. [PDF]
Booth H, Ma W, Karakuş O.
europepmc +1 more source
The photometric variability of massive stars due to gravity waves excited by core convection. [PDF]
Anders EH+10 more
europepmc +1 more source
A helium-burning white dwarf binary as a supersoft X-ray source. [PDF]
Greiner J+14 more
europepmc +1 more source
Color-Magnitude Arrays for Two Associations in the Large Magellanic Cloud.
Bart J. Bok, P. F. Bok, J. M. Basinski
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