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HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE): The Large Magellanic Cloud dust
(2010)
The HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) of the Magellanic Clouds will use dust emission to investigate the life cycle of matter in both the Large and Small Magellanic Clouds (LMC and SMC). Using ...
Detection of an ultra-bright submillimeter galaxy behind the small magellanic cloud*
(The Astrophysical Journal Letters, 2013)
The Relationship Between Molecular GAS, H I, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds
(2016)
The Magellanic Clouds provide the only laboratory to study the effects of metallicity and galaxy mass on molecular gas and star formation at high (similar to 20 pc) resolution. We use the dust emission from HERITAGE Herschel ...
The VISCACHA survey-II. Structure of star clusters in the Magellanic Clouds periphery
(Oxford University Press, 2020-10)
We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters' stellar density and surface brightness ...
On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
(Wiley, 2013-10)
We model the dynamical interaction between the Small and LargeMagellanic Clouds and their corresponding stellar cluster populations. Our goal is to explore whether the lack of old clusters (>7 Gyr) in the Small Magellanic ...
Results of the ESO-SEST key programme: CO in the Magellanic Clouds VI. The 30 Doradus Complex
(Editions Physique, 1997-04)
We report observations of 12CO(1 ! 0) emission
from molecular clouds in a complex extending 2 kpc
south of 30 Dor in the Large Magellanic Cloud. The observations
were taken on the Swedish-ESO Submillimetre
Telescope ...
Background galaxies as reddening probes throughout the Magellanic Clouds
(EDP Sciences, 2001-06)
We study the spectral properties in the range 3600 Å-6800 Å of the nuclear region of galaxies behind the Magellanic Clouds. The radial velocities clarified the nature of the objects as background galaxies or extended objects ...
The age-metallicity relationship in the Small Magellanic Cloud periphery
(Wiley Blackwell Publishing, Inc, 2015-05)
We present results from Washington CT1 photometry for 11 star fields located in the western outskirts of the Small Magellanic Cloud (SMC), which cover angular distances to its centre from 2° up to 13° (≈2.2-13.8 kpc). The ...
Submillimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution
(Astronomy and Astrophysics, 2010)