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Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 552, p. A121
Context. The self-enrichment scenario for globular clusters (GC) requires large amounts of residual gas after the initial formation of the first stellar generation... 
ISM: jets and outflows | ISM: bubbles | Globular clusters: general | ABUNDANCE PATTERNS | MOLECULAR CLOUDS | 1ST STARS | MAIN-SEQUENCE | BLACK-HOLES | 2 STELLAR POPULATIONS | ORIGIN | EVOLUTION | globular clusters: general | ASTRONOMY & ASTROPHYSICS | MULTIPLE POPULATIONS | GALACTIC-CENTER
Journal Article
Nature, ISSN 0028-0836, 12/2012, Volume 492, Issue 7428, pp. 221 - 224
The formation of very wide binary systems(1-3), such as the a Centauri system with Proxima... 
EVOLUTION | CATALOG | HIPPARCOS STARS | MULTIDISCIPLINARY SCIENCES | PROPER MOTION | TERTIARY COMPANIONS | CLUSTER | DISK | Evolution | Research | Star formation | Galaxies | Observations | Stars, Double | Collapsing | Clouds | Dynamics | Stars | Clusters | Binary systems | Orbits | Dynamical systems
Journal Article
2011, Environmental science, engineering and technology, ISBN 1612095275, 120
Book
The Astrophysical journal, ISSN 1538-4357, 2018, Volume 859, Issue 2, p. 151
Magnetic field plays a crucial role in shaping molecular clouds and regulating star formation, yet the complete information on the magnetic field is not well constrained owing to the limitations in observations... 
stars: formation | ISM: clouds | ISM: magnetic fields | CLUMP IDENTIFICATION | MOLECULAR CLOUDS | DUST EMISSION | TURBULENT | FRAGMENTATION | SCUBA-2 | ASTRONOMY & ASTROPHYSICS | ACCRETION | SIMULATIONS | POLARIZATION | KINEMATICS | Turbulence | Accretion | Turbulent flow | Clouds | Fluid dynamics | Molecular clouds | Field strength | Ammonia | Star formation | Gravitational collapse | Clumps | Magnetism | Cloud formation | Magnetic fields | Star & galaxy formation | Deposition
Journal Article
The Astrophysical journal, ISSN 1538-4357, 2018, Volume 854, Issue 1, p. 16
The Kennicutt-Schmidt (KS) relationship between the surface density of the star formation rate (SFR... 
stars: formation | ISM: molecules | galaxies: ISM | galaxies: star formation | local interstellar matter | MOLECULAR CLOUDS | SPIRAL GALAXIES | JCMT NEARBY GALAXIES | GAS-SURFACE-DENSITY | FORMATION EFFICIENCY | G