KINEMATIC STRUCTURE OF MOLECULAR GAS AROUND HIGH-MASS YSO, PAPILLON NEBULA, IN N159 EAST IN THE LARGE MAGELLANIC CLOUD: A NEW PERSPECTIVE WITH ALMA [PDF]
, 2016 We present the ALMA Band 3 and Band 6 results of 12CO(2-1), 13CO(2-1), H30α recombination line, free–free emission around 98 GHz, and the dust thermal emission around 230 GHz toward the N159 East Giant Molecular Cloud (N159E) in the Large Magellanic ...
K. Saigo +22 more
semanticscholar +1 more source
A Strange Mènage Á Trois [PDF]
arXiv, 2010 The Magellanic Clouds may have joined our Milky Way system quite recently. The Large Magellanic Cloud turns out to be a remarkably luminous object that is close to the upper luminosity limit of the class of magellanic irregular galaxies.
arxiv
LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW [PDF]
, 2014 We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope.
L. Macri +4 more
semanticscholar +1 more source
Cosmic Ray Accelerators in the Large Magellanic Cloud [PDF]
, 2010 I point out a correlation between gamma-ray emissivity and the historical star formation rate in the Large Magellanic Cloud ~12.5 Myr ago. This correlation bolsters the view that CRs in the LMC are accelerated by conglomerations of supernova remnants: i.e. superbubbles and supergiant shells.
arxiv +1 more source
A DIPOLE ON THE SKY: PREDICTIONS FOR HYPERVELOCITY STARS FROM THE LARGE MAGELLANIC CLOUD [PDF]
, 2016 We predict the distribution of hypervelocity stars (HVSs) ejected from the Large Magellanic Cloud (LMC), under the assumption that the dwarf galaxy hosts a central massive black hole (MBH).
D. Boubert, N. W. Evans
semanticscholar +1 more source
The chemical composition of the Small Magellanic Cloud [PDF]
, 2013 The Small Magellanic Cloud is a close, irregular galaxy that has experienced a complex star formation history due to the strong interactions occurred both with the Large Magellanic Cloud and the Galaxy. Despite its importance, the chemical composition of its stellar populations older than 1-2 Gyr is still poorly investigated.
arxiv +1 more source
ALMA Observations of a Quiescent Molecular Cloud in the Large Magellanic Cloud [PDF]
, 2017 We present high-resolution (subparsec) observations of a giant molecular cloud in the nearest star-forming galaxy, the Large Magellanic Cloud. ALMA Band 6 observations trace the bulk of the molecular gas in 12CO(2–1) and the high column density regions ...
T. Wong +21 more
semanticscholar +1 more source
An H I Aperture Synthesis Mosaic of the Large Magellanic Cloud
, 1998 We present the results of an H I aperture synthesis mosaic of the Large Magellanic Cloud (LMC), made by combining data from 1344 separate pointing centers using the Australia Telescope Compact Array (ATCA). The resolution of the mosaicked images is 1.′0 (
Sungeun Kim +6 more
semanticscholar +1 more source
Supernova Remnants In The Magellanic Clouds [PDF]
arXiv, 2016 We present initial results of an ongoing study of the supernova remnants (SNRs) and candidates in the Magellanic Clouds. Some 108 objects in both Clouds are considered to be either an SNR or a reliable candidate. This represents the most complete sample of known SNRs in any galaxy. therefore, this study allows us to study SNR population properties such
arxiv
THE MAGELLANIC CLOUDS. XV. ON THE TILT OF THE LARGE CLOUD [PDF]
, 1955 Virginia McKibben Nail, Harlow Shapley
openalex +1 more source