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The molecular gas content of blue dwarf galaxies A collapsing detached molecular system in He 2-10?
(EDP SCIENCES S A, 2009)
We present new observations of a sample of blue dwarf galaxies in the lines of CO(3-2) and HCN(4-3). The observations were obtained with the 12 m APEX telescope located at an altitude of 5100 m in Chajnantor (ALMA site). ...
A complete CO survey of the Large Magellanic Cloud
(1988-08-15)
A complete CO survey of the central 6 deg x 6 deg of the LMC was performed in order to determine the distribution of molecular clouds. At least 10 percent of the region studied exhibits CO line emission, with peak line ...
The star cluster frequency throughout the Large Magellanic Cloud
(Wiley Blackwell Publishing, Inc, 2014-01)
We address the issue of the variation in star cluster frequency (CF) in the Large Magellanic Cloud (LMC) in terms of cluster spatial distribution. We adopt the LMC regions traced by Harris & Zaritsky and use an updated ...
An analysis of the population of extended main sequence turn-off clusters in the Large Magellanic Cloud
(Wiley Blackwell Publishing, Inc, 2016-12)
We combine a number of recent studies of the extended main sequence turn-off (eMSTO) phenomenon in intermediate age stellar ($1-2$~Gyr) clusters in the Large Magellanic Cloud (LMC) in order to investigate its origin. By ...
Dust in the Small Magellanic Cloud
(Combes, F.Barret, D., 2004)
The Small Magellanic Cloud is a nearby galaxy of low metallicity, strong star formation rate in spite of an apparently small proportion of molecular gas (weak and rare CO detections). The observations of gas and dust of ...
Exploring the Very Extended Low-surface-brightness Stellar Populations of the Large Magellanic Cloud with SMASH
(Institute of Physics Publishing, 2019)
We present the detection of very extended stellar populations around the Large Magellanic Cloud (LMC) out to R ∼ 21°, or ∼18.5 kpc at the LMC distance of 50 kpc, as detected in the Survey of the Magellanic Stellar History ...
A (C-12)O survey of the Small Magellanic Cloud
(1991-02-10)
The central 2 arcsec x 2 arcsec region of the SMC has been fully surveyed to search for (C-12)O emission in the J = 1-0 transition. (C-12)O emission from two large complexes located in the southwest and northeast regions ...
Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
(EDP Sciences, 2017-06)
Aims. We seek to produce a homogeneous catalog of astrophysical parameters of 239 resolved star clusters, located in the Small and Large Magellanic Clouds, observed in the Washington photometric system. Methods. The cluster ...