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
Observation of a neutrino burst in coincidence with supernova 1987A in the Large Magellanic Cloud.
R. Bionta +36 more
semanticscholar +1 more source
Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S +7 more
europepmc +1 more source
High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm [PDF]
Roya Hamedani Golshan +6 more
openalex +1 more source
PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF MASSIVE BINARIES IN THE LARGE MAGELLANIC CLOUD. II. THREE O-TYPE SYSTEMS IN THE 30 Dor REGION [PDF]
N. Morrell +4 more
openalex +1 more source
Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (SAGE)
M. Meixner +16 more
semanticscholar +1 more source
Young star clusters immersed in intermediate-age fields in the Large Magellanic Cloud bar [PDF]
Andrés E. Piatti +3 more
openalex +1 more source
Cluster formation versus star formation rates around sixregions in the Large Magellanic Cloud [PDF]
Annapurni Subramaniam
openalex +1 more source
The infall of the Large Magellanic Cloud (LMC) into the Milky Way’s halo impacts the distribution of stars and dark matter (DM) in our Galaxy. Mapping the observational consequences of this encounter can inform us about the properties of both galaxies ...
Manuel Cavieres +8 more
doaj +1 more source

