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1. Full Text The Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN. I. Catalog of Molecular Clouds
by Fukui, Y and Kawamura, A and Minamidani, T and Mizuno, Y and Kanai, Y and Mizuno, N and Onishi, T and Yonekura, Y and Mizuno, A and Ogawa, H and Rubio, M
The Astrophysical Journal Supplement Series, ISSN 0067-0049, 09/2008, Volume 178, Issue 1, pp. 56 - 70
The second survey of the molecular clouds in the Large Magellanic Cloud in (CO)-C-12 (J = 1-0) was carried out by NANTEN. The sensitivity of this survey is... 
Magellanic clouds | Stars: Formation | ISM: Structure | Galaxies: ISM | ISM: Molecules | Radio lines: ISM | STELLAR CLUSTERS | LOCAL GROUP | 1ST GALACTIC QUADRANT | NEUTRAL HYDROGEN | STAR-FORMATION | CO SURVEY | ISM: structure | GIANT | stars: formation | RADIO-CONTINUUM | radio lines: ISM | ISM: molecules | galaxies: ISM | SEST KEY PROGRAM | ASTRONOMY & ASTROPHYSICS | Magellanic Clouds | FAR-INFRARED EMISSION | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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2. Full Text The turbulent destruction of clouds - III. Three-dimensional adiabatic shock-cloud simulations
by Pittard, J.M and Parkin, E.R
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2016, Volume 457, Issue 4, pp. 4470 - 4498
We present 3D hydrodynamic simulations of the adiabatic interaction of a shock with a dense, spherical cloud. We compare how the nature of the interaction... 
Shock waves | ISM: supernova remnants | Turbulence | hydrodynamics | ISM: clouds | ISM: kinematics and dynamics | INTERSTELLAR GAS CLOUDS | STAR-FORMING GALAXIES | turbulence | X-RAY SPECTROSCOPY | MACH NUMBER DEPENDENCE | SUPER-NOVA REMNANT | STRIPPED ELLIPTIC GALAXIES | SPACE-TELESCOPE OBSERVATIONS | ASTRONOMY & ASTROPHYSICS | MASS INJECTION RATES | LARGE-MAGELLANIC-CLOUD | COLLIDING WINDS | shock waves | Physics - Astrophysics of Galaxies
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3. Full Text The formation and destruction of molecular clouds and galactic star formation: An origin for the cloud mass function and star formation efficiency
by Inutsuka, Shu-Ichiro and Inoue, Tsuyoshi and Iwasaki, Kazunari and Hosokawa, Takashi
Astronomy and Astrophysics, ISSN 0004-6361, 08/2015, Volume 580, p. A49
We describe an overall picture of galactic-scale star formation. Recent high-resolution magneto-hydrodynamical simulations of two-fluid dynamics with cooling,... 
ISM: clouds | Stars: formation | ISM: bubbles | ISM: structure | ISM: kinematics and dynamics | ISM: magnetic fields | GAS DEPLETION TIME | MAGNETOHYDRODYNAMIC SIMULATIONS | DISSOCIATION FRONT | FORMATION RATES | DYNAMICAL EXPANSION | stars: formation | GSH 277+00+36 | H I FLOWS | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | LARGE-MAGELLANIC-CLOUD | ACCRETION FLOWS | Clouds | Destruction | Exponents | Star formation | Simulation | Molecular clouds | Time | Formations
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4. The Magellanic clouds
: A European Southern Observatory presentation: principal prospects, current observational and theoretical approaches, and prospects for future research. Based on the Symposium on the Magellanic Clouds, held in Santiago de Chile, March 1969, on the occasion of the dedication of the European Southern Observatory. Ed. by André B. Muller
by Symposium on the Magellanic Clouds, Santiago, 1969 and Muller, André B and European Southern Observatory
1971, Astrophysics and space science library, v. 23, Volume 23, xii, 189 p. illus.
Magellanic Clouds Congresses
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5. Full Text Discovery of Shocked Molecular Clouds Associated with the Shell-type Supernova Remnant RX J0046.5-7308 in the Small Magellanic Cloud
by Sano, H and Matsumura, H and Yamane, Y and Maggi, P and Fujii, K and Tsuge, K and Tokuda, K and Alsaberi, RZE and Filipovic, MD and Maxted, N and Rowell, G and Uchida, H and Tanaka, T and Muraoka, K and Takekoshi, T and Onishi, T and Kawamura, A and Minamidani, T and Mizuno, N and Yamamoto, H and Tachihara, K and Inoue, T and Inutsuka, S and Voisin, F and Tothill, NFH and Sasaki, M and McClure-Griffiths, NM and Fukui, Y
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 08/2019, Volume 881, Issue 1, p. 85
RX J0046.5-7308 is a shell-type supernova remnant (SNR) in the Small Magellanic Cloud (SMC). We carried out new (CO)-C-12(J = 1-0, 3-2) observations toward the... 
INTERSTELLAR GAS | ISM: supernova remnants | TELESCOPE | H-I | RADIATIVE-TRANSFER | ATCA RADIO-CONTINUUM | GAMMA-RAY EMISSION | MODELS | ISM: individual objects (RX J0046.5-7308, DEM S23) | SEST KEY PROGRAM | ASTRONOMY & ASTROPHYSICS | X-RAY | Magellanic Clouds | ISM: clouds
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6. The Magellanic Clouds
by Westerlund, Bengt E and Westerlund, B. E
1997, Cambridge astrophysics series, ISBN 0521480701, Volume 29., xv, 279
The Magellanic Clouds – a pair of nearby, satellite galaxies – are caught in a dynamic struggle internally and with our Milky Way. Given their close proximity,... 
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7. Full Text A comparative study of giant molecular clouds in M51, M33, and the large magellanic cloud
by Hughes, Annie and Meidt, Sharon E and Colombo, Dario and Schinnerer, Eva and Pety, Jerôme and Leroy, Adam K and Dobbs, Clare L and García-Burillo, Santiago and Thompson, Todd A and Dumas, Gaëlle and Schuster, Karl F and Kramer, Carsten
Astrophysical Journal, ISSN 0004-637X, 12/2013, Volume 779, Issue 1, pp. 46 - 20
We compare the properties of giant molecular clouds (GMCs) in M51 identified by the Plateau de Bure Interferometer Whirlpool Arcsecond Survey with GMCs... 
ISM: clouds | galaxies: individual (M51, M33, Large Magellanic Cloud) | ISM: molecules | galaxies: ISM | ISM: structure | NEARBY GALAXIES | LOCAL GROUP | VELOCITY DISPERSION | H-I | ON SPIRAL GALAXIES | STAR-FORMATION | CO-TO-H-2 CONVERSION FACTOR | INTERSTELLAR-MEDIUM | ALL-DISK SURVEY | ASTRONOMY & ASTROPHYSICS | DWARF SEYFERT NUCLEI | Magellanic clouds | Populations | Molecular clouds | Emissions control | Dispersions | Carbon monoxide | Density | Interstellar matter | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | VARIATIONS | DISPERSIONS | RESOLUTION | CORRELATIONS | COMPARATIVE EVALUATIONS | CARBON MONOXIDE | MOLECULES | DENSITY | INTERFEROMETERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | GALAXIES | EMISSION | MAGELLANIC CLOUDS | SURFACES
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8. Full Text Swift Ultraviolet Survey of the Magellanic Clouds (SUMaC) – I. Shape of the ultraviolet dust extinction law and recent star formation history of the Small Magellanic Cloud
by Hagen, Lea M. Z and Siegel, Michael H and Hoversten, Erik A and Gronwall, Caryl and Immler, Stefan and Hagen, Alex
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2016, Volume 466, Issue 4, pp. 4540 - 4557
Abstract We present the first results from the Swift Ultraviolet Survey of the Magellanic Clouds, the highest resolution ultraviolet (UV) survey of the... 
ULTRA-VIOLET/OPTICAL TELESCOPE | CALIBRATION | MOLECULAR CLOUDS | SIMILAR-TO 2 | INFRARED EXTINCTION | galaxies: individual: SMC | INTERSTELLAR EXTINCTION | dust, extinction | EVOLUTION | FORMING GALAXIES | ASTRONOMY & ASTROPHYSICS | Magellanic Clouds | STELLAR POPULATIONS | MILKY-WAY | Physics - Astrophysics of Galaxies
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9. Full Text Molecular Clouds in the Milky Way
by Heyer, Mark and Dame, T.M
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 8/2015, Volume 53, Issue 1, pp. 583 - 629
In the past twenty years, the reconnaissance of 12 CO and 13 CO emission in the Milky Way by single-dish millimeter-wave telescopes has expanded our view and... 
molecules; radio lines: ISM | Galaxy: disk | kinematics and dynamics | structure; ISM: clouds | Molecules; radio lines: ISM | Structure; ISM: clouds | Kinematics and dynamics | PRINCIPAL COMPONENT ANALYSIS | LARGE-SCALE STRUCTURE | CO J=2-1 SURVEY | STAR-FORMING REGIONS | GALACTIC PLANE SURVEY | DENSE INTERSTELLAR CLOUDS | radio lines: ISM | GAMMA-RAY EMISSION | ASTRONOMY & ASTROPHYSICS | Galaxy: disk, structure | ISM: clouds, kinematics and dynamics, molecules | PHOTON-DOMINATED REGIONS | INITIAL MASS FUNCTION | LARGE-MAGELLANIC-CLOUD | Clouds | Observations | Milky Way | Molecular clouds
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10. Full Text Modelling CO emission - I. CO as a column density tracer and the X factor in molecular clouds
by Shetty, Rahul and Glover, Simon C and Dullemond, Cornelis P and Klessen, Ralf S
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2011, Volume 412, Issue 3, pp. 1686 - 1700
Theoretical and observational investigations have indicated that the abundance of carbon monoxide (CO) is very sensitive to intrinsic properties of the gaseous... 
stars: formation | ISM: clouds | methods: numerical | ISM: molecules | ISM: structure