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Astrochemistry and compositions of planetary systems
Planets form and obtain their compositions in disks of gas and dust around young stars. The
chemical compositions of these planet-forming disks regulate all aspects of planetary …
chemical compositions of these planet-forming disks regulate all aspects of planetary …
Complex organic interstellar molecules
Of the over 150 different molecular species detected in the interstellar and circumstellar
media, approximately 50 contain 6 or more atoms. These molecules, labeled complex by …
media, approximately 50 contain 6 or more atoms. These molecules, labeled complex by …
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 …
The SILCC (SImulating the LifeCycle of molecular Clouds) project–I. Chemical evolution of the supernova-driven ISM
Abstract The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …
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 …
The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function
Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …
generation of radiant energy, synthesis of elements, formation of planets, and development …
Cold dark clouds: the initial conditions for star formation
EA Bergin, M Tafalla - Annu. Rev. Astron. Astrophys., 2007 - annualreviews.org
Cold dark clouds are nearby members of the densest and coldest phase in the Galactic
interstellar medium, and represent the most accessible sites where stars like our Sun are …
interstellar medium, and represent the most accessible sites where stars like our Sun are …
Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region
Context. Core condensation is a critical step in the star-formation process, but it is still poorly
characterized observationally. Aims. We have studied the 10 pc-long L1495/B213 complex …
characterized observationally. Aims. We have studied the 10 pc-long L1495/B213 complex …
Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
We present Phantom, a fast, parallel, modular, and low-memory smoothed particle
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
The molecular cloud lifecycle
M Chevance, JMD Kruijssen… - Space Science …, 2020 - Springer
Giant molecular clouds (GMCs) and their stellar offspring are the building blocks of galaxies.
The physical characteristics of GMCs and their evolution are tightly connected to galaxy …
The physical characteristics of GMCs and their evolution are tightly connected to galaxy …