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]
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
The Dark Energy Camera Magellanic Clouds Emission-line Survey
We have used the Dark Energy Camera (DECam) on the CTIO Blanco 4 m telescope to perform a new emission-line survey of the Large Magellanic Cloud (LMC) using narrowband H α and [S ii ] filters in addition to a continuum band to create pure emission-line ...
Sean D. Points +9 more
doaj +1 more source
LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW [PDF]
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
The Truncated Circumgalactic Medium of the Large Magellanic Cloud
The Large Magellanic Cloud (LMC) is the nearest massive galaxy to the Milky Way (MW). Its circumgalactic medium (CGM) is complex and multiphase, containing both stripped H i structures like the Magellanic Stream and Bridge and a diffuse warm corona seen ...
Sapna Mishra +8 more
doaj +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
LMC-driven Anisotropic Boosts in Stream–Subhalo Interactions
Dark matter subhalos are predicted to perturb stellar streams; stream morphologies and dynamics can, therefore, constrain the mass distribution of subhalos.
Arpit Arora +6 more
doaj +1 more source
LOOKING OUTSIDE THE GALAXY: THE DISCOVERY OF CHEMICAL ANOMALIES IN THREE OLD LARGE MAGELLANIC CLOUD CLUSTERS [PDF]
A. Mucciarelli +3 more
openalex +1 more source
NGC 1856: Using Machine Learning Techniques to Uncover Detailed Stellar Abundances from MUSE Data
We present the first application of the novel approach based on data-driven machine learning methods applied to Multi-Unit Spectroscopic Explorer (MUSE) field data to derive stellar abundances of star clusters.
Randa Asa’d +7 more
doaj +1 more source
Carbonaceous dust grains seen in the first billion years of cosmic time. [PDF]
Witstok J +41 more
europepmc +1 more source
The Gaseous Blowout of the 30 Doradus Starburst Region in the LMC
Widespread galactic winds emanate from the Large Magellanic Cloud (LMC), with the 30 Doradus starburst region generating the fastest and most concentrated gas flows.
Suraj Poudel +22 more
doaj +1 more source

