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From filamentary networks to dense cores in molecular clouds: toward a new paradigm for star formation
P André, J Di Francesco… - … and Planets VI, 2014 - books.google.com
Recent studies of the nearest star-forming clouds of the Galaxy at submillimeter wavelengths
with the Herschel Space Observatory have provided us with unprecedented images of the …
with the Herschel Space Observatory have provided us with unprecedented images of the …
Theory of star formation
We review current understanding of star formation, outlining an overall theoretical framework
and the observations that motivate it. A conception of star formation has emerged in which …
and the observations that motivate it. A conception of star formation has emerged in which …
Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario
We present a unified description of the scenario of global hierarchical collapse (GHC). GHC
constitutes a flow regime of (non-homologous) collapses within collapses, in which all …
constitutes a flow regime of (non-homologous) collapses within collapses, in which all …
[HTML][HTML] 3D turbulent reconnection: Theory, tests, and astrophysical implications
Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …
magnetized plasmas. It is associated with energy release in regions of magnetic field …
Control of star formation by supersonic turbulence
Understanding the formation of stars in galaxies is central to much of modern astrophysics.
However, a quantitative prediction of the star formation rate and the initial distribution of …
However, a quantitative prediction of the star formation rate and the initial distribution of …
The physics of star cluster formation and evolution
Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is
transformed to turbulence with stars forming from cores fed by filaments. In the most compact …
transformed to turbulence with stars forming from cores fed by filaments. In the most compact …
Planck intermediate results-XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
PAR Ade, N Aghanim, MIR Alves, M Arnaud… - Astronomy & …, 2016 - aanda.org
Within ten nearby (d< 450 pc) Gould belt molecular clouds we evaluate statistically the
relative orientation between the magnetic field projected on the plane of sky, inferred from …
relative orientation between the magnetic field projected on the plane of sky, inferred from …
Toward understanding massive star formation
Although fundamental for astrophysics, the processes that produce massive stars are not
well understood. Large distances, high extinction, and short timescales of critical …
well understood. Large distances, high extinction, and short timescales of critical …
Interstellar turbulence I: observations and processes
▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density
regimes in the interstellar gas. This two-part review summarizes the observations, theory …
regimes in the interstellar gas. This two-part review summarizes the observations, theory …
Turbulent molecular clouds
Stars form within molecular clouds but our understanding of this fundamental process
remains hampered by the complexity of the physics that drives their evolution. We review our …
remains hampered by the complexity of the physics that drives their evolution. We review our …