Molecular clouds in nearby galaxies
Y Fukui, A Kawamura - Annual Review of Astronomy and …, 2010 - annualreviews.org
We present a review of spatially resolved giant molecular clouds (GMCs) in nearby galaxies,
aiming at providing a template of GMC properties, which may be extrapolated to distant …
aiming at providing a template of GMC properties, which may be extrapolated to distant …
Unbound young stellar systems: star formation on the loose
DA Gouliermis - Publications of the Astronomical Society of the …, 2018 - iopscience.iop.org
Unbound young stellar systems, the loose ensembles of physically related young bright
stars, trace the typical regions of recent star formation in galaxies. Their morphologies vary …
stars, trace the typical regions of recent star formation in galaxies. Their morphologies vary …
Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large Magellanic Cloud
AD Mackey⋆, GF Gilmore - Monthly Notices of the Royal …, 2003 - academic.oup.com
We have compiled a pseudo-snapshot data set of two-colour observations from the Hubble
Space Telescope archive for a sample of 53 rich LMC clusters with ages of 106–1010 yr. We …
Space Telescope archive for a sample of 53 rich LMC clusters with ages of 106–1010 yr. We …
The origin of the magellanic stream and its leading arm
DL Nidever, SR Majewski… - The Astrophysical Journal, 2008 - iopscience.iop.org
ABSTRACT We explore the Magellanic Stream (MS) using a Gaussian decomposition of the
H i velocity profiles in the Leiden-Argentine-Bonn (LAB) all-sky H i survey. This …
H i velocity profiles in the Leiden-Argentine-Bonn (LAB) all-sky H i survey. This …
The IRSF Magellanic Clouds point source catalog
D Kato, C Nagashima, T Nagayama… - Publications of the …, 2007 - academic.oup.com
We present a near-infrared () photometric catalog, including 14811185 point sources for a
40 deg area of the Large Magellanic Cloud, 2769682 sources for an 11 deg area of the …
40 deg area of the Large Magellanic Cloud, 2769682 sources for an 11 deg area of the …
The optical depth of H ii regions in the Magellanic Clouds
EW Pellegrini, MS Oey, PF Winkler… - The Astrophysical …, 2012 - iopscience.iop.org
We exploit ionization-parameter mapping (IPM) as a powerful tool to measure the optical
depth of star-forming H ii regions. Our simulations using the photoionization code Cloudy …
depth of star-forming H ii regions. Our simulations using the photoionization code Cloudy …
A general catalogue of extended objects in the Magellanic System
Abstract We update the Small Magellanic Cloud (SMC), Bridge and Large Magellanic Cloud
(LMC) catalogues of extended objects that were constructed by members of our group from …
(LMC) catalogues of extended objects that were constructed by members of our group from …
The VLT-FLAMES Tarantula Survey-XXIX. Massive star formation in the local 30 Doradus starburst
FRN Schneider, OH Ramírez-Agudelo… - Astronomy & …, 2018 - aanda.org
The 30 Doradus (30 Dor) nebula in the Large Magellanic Cloud (LMC) is the brightest HII
region in the Local Group and a prototype starburst similar to those found in high redshift …
region in the Local Group and a prototype starburst similar to those found in high redshift …
A Multi-band Catalog of 10978 Star Clusters, Associations, and Candidates in the Milky Way
E Bica, DB Pavani, CJ Bonatto… - The Astronomical …, 2018 - iopscience.iop.org
We present a catalog of Galactic star clusters, associations and candidates with 10978
entries. This multi-band catalog was constructed over 20 years, starting with visual …
entries. This multi-band catalog was constructed over 20 years, starting with visual …
Ca II triplet spectroscopy of Large Magellanic Cloud red giants. I. Abundances and velocities for a sample of populous clusters
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared
spectra for more than 200 stars in 28 populous LMC clusters. This cluster sample spans a …
spectra for more than 200 stars in 28 populous LMC clusters. This cluster sample spans a …