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February 2023 |
The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks
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June 2009 |
Synthetic CO emission and the XCO factor of young molecular clouds: a convergence study
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November 2021 |
The Dynamics of Low‐Mass Molecular Clouds in External Radiation Fields
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June 1997 |
A New Numerical Scheme for Cosmic-Ray Transport
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February 2018 |
On the low ortho-to-para H2 ratio in star-forming filaments
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October 2021 |
Three-phase Interstellar Medium in Galaxies Resolving Evolution with Star Formation and Supernova Feedback (TIGRESS): Algorithms, Fiducial Model, and Convergence
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September 2017 |
The X CO Conversion Factor from Galactic Multiphase ISM Simulations
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April 2018 |
grackle: a chemistry and cooling library for astrophysics
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December 2016 |
The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM
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September 2015 |
An Extension of the Athena++ Framework for General Equations of State
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April 2020 |
KROME - a package to embed chemistry in astrophysical simulations
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February 2014 |
Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS‐MP
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July 2006 |
The UMIST database for astrochemistry 2012
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January 2013 |
Global Simulations of Protoplanetary Disk Outflows with Coupled Non-ideal Magnetohydrodynamics and Consistent Thermochemistry
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March 2019 |
Modeling UV Radiation Feedback from Massive Stars. I. Implementation of Adaptive Ray-tracing Method and Tests
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December 2017 |
Dissociative recombination of rotationally coldH3+
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November 2004 |
Enzo: an Adaptive mesh Refinement code for Astrophysics
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March 2014 |
Simulating the formation of massive seed black holes in the early Universe – I. An improved chemical model
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June 2015 |
Simulating the Formation of Molecular Clouds. I. Slow Formation by Gravitational Collapse from Static Initial Conditions
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April 2007 |
Chemistry and radiative shielding in star-forming galactic discs
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October 2016 |
Cosmic-Ray Transport in Simulations of Star-forming Galactic Disks
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November 2021 |
The Millennium Arecibo 21 Centimeter Absorption‐Line Survey. II. Properties of the Warm and Cold Neutral Media
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April 2003 |
Modelling CO formation in the turbulent interstellar medium
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April 2010 |
Athena: A New Code for Astrophysical MHD
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September 2008 |
On the Stability and Evolution of Isolated Bok Globules
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October 1999 |
Uncertainties in H 2 and HD chemistry and cooling and their role in early structure formation
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August 2008 |
The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers
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June 2020 |
Diffuse Ionized Gas in Simulations of Multiphase, Star-forming Galactic Disks
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July 2020 |
Cosmological hydrodynamics with adaptive mesh refinement: A new high resolution code called RAMSES
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April 2002 |
Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas
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November 2008 |
The neutral atomic phases of the interstellar medium
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April 1995 |
FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes
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November 2000 |
Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
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December 2022 |
Structure of Stationary Photodissociation Fronts
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September 1996 |
TIGRESS simulation data
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dataset
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January 2022 |
Photodissociation regions. I - Basic model. II - A model for the Orion photodissociation region
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April 1985 |
Photoelectric heating of interstellar gas
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April 1978 |
The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks
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January 2007 |
Physics of the Interstellar and Intergalactic Medium
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book
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December 2011 |
\documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{H}\,^{+}_{3}$ \end{document} in Diffuse Interstellar Clouds: A Tracer for the Cosmic‐Ray Ionization Rate
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December 2007 |
Metallicity Dependence of the H/H2 and C+/C/CO Distributions in a Resolved Self-regulating Interstellar Medium
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October 2021 |
CVODE, A Stiff/Nonstiff ODE Solver in C
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January 1996 |
Evaporation of Low-mass Planet Atmospheres: Multidimensional Hydrodynamics with Consistent Thermochemistry
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June 2018 |
A new class of accurate, mesh-free hydrodynamic simulation methods
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April 2015 |
Introducing TIGRESS-NCR. I. Coregulation of the Multiphase Interstellar Medium and Star Formation Rates
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March 2023 |
Reaction Networks for Interstellar Chemical Modelling: Improvements and Challenges
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October 2010 |
Molecular Depletion and Thermal Balance in Dark Cloud Cores
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August 2001 |
A chemical reaction network solver for the astrophysics code NIRVANA
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January 2016 |
A Simple and Accurate Network for Hydrogen and Carbon Chemistry in the Interstellar Medium
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June 2017 |
Cosmic-Ray Transport in Varying Galactic Environments
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April 2022 |
The Environmental Dependence of the X CO Conversion Factor
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November 2020 |