Results 131 to 140 of about 609,374 (282)
The Proper Motion of the Large Magellanic Cloud: A Reanalysis [PDF]
The Astronomical Journal, 2006 Accepted for publication in ...
M.H. Pedreros +5 more
openaire +3 more sources
A 10 kpc stellar substructure at the edge of the Large Magellanic Cloud: Perturbed outer disc or evidence for tidal stripping? [PDF]
, 2015 We report the discovery of a substantial stellar overdensity in the periphery of the Large Magellanic Cloud (LMC), found using public imaging from the first year of the Dark Energy Survey.
D. Mackey +5 more
semanticscholar +1 more source
The exceptionally powerful TeV γ-ray emitters in the Large Magellanic Cloud [PDF]
Science, 2015 A light on the origin of cosmic rays There's a new lab for studying the origins of cosmic rays: our neighbor galaxy, the Large Magellanic Cloud. Astronomers are now making progress on this topic by examining the gamma rays that are produced when cosmic ...
H. C. A. Abramowski +226 more
semanticscholar +1 more source
The Astronomical JournalSupergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy’s halo. The SGSs in the Large Magellanic Cloud (LMC) are so close that their stars can be resolved with ground-based telescopes to ...
Po-Sheng Ou +4 more
doaj +1 more source
The Astrophysical Journal, 2023 In the context of a project aimed at characterizing the dynamical evolution of old globular clusters in the Large Magellanic Cloud, we have secured deep HST/WFC3 images of the massive cluster NGC 1835.
Camilla Giusti +8 more
doaj +1 more source
The Magellanic Clouds, Past, Present and Future - A Summary of IAU Symposium No. 190 [PDF]
arXiv, 1998 Important problems to which we would like to find answers are: What are the distances to the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC)? What is the present distribution of stars, gas and dark matter in the Clouds, and how did it evolve?
arxiv
THE CHEMICAL ENRICHMENT HISTORY OF THE LARGE MAGELLANIC CLOUD [PDF]
The Astronomical Journal, 2008 Ca II triplet spectroscopy has been used to derive stellar metallicities for individual stars in four LMC fields situated at galactocentric distances of 3\arcdeg, 5\arcdeg, 6\arcdeg\@ and 8\arcdeg\@ to the north of the Bar. Observed metallicity distributions show a well defined peak, with a tail toward low metallicities.
Eduardo Hardy +6 more
openaire +5 more sources
A LUMINOUS GAMMA-RAY BINARY IN THE LARGE MAGELLANIC CLOUD [PDF]
, 2016 Gamma-ray binaries consist of a neutron star or a black hole interacting with a normal star to produce gamma-ray emission that dominates the radiative output of the system.
R. Corbet +11 more
semanticscholar +1 more source
Morphology of stellar populations in the Magellanic Clouds using the VMC survey [PDF]
arXiv, 2018 The Magellanic Clouds are nearby dwarf irregular galaxies that represent a unique laboratory for studying galaxy interactions. Their morphology and dynamics have been heavily influenced by their mutual interactions as well as with their interaction(s) with the Milky Way.
arxiv
Deep view of the Large Magellanic Cloud with six years of Fermi -LAT observations [PDF]
, 2015 The nearby Large Magellanic Cloud (LMC) provides a rare opportunity of a spatially resolved view of an external star-forming galaxy in gamma-rays. The LMC was detected at 0.1-100GeV as an extended source with CGRO/EGRET and using early observations with ...
M. Ackermann +103 more
semanticscholar +1 more source