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The efficiency of grain growth in the diffuse interstellar medium
Free accessBASE | 2021|Keywords: ISM: evolution -
A new radiative cooling curve based on an up-to-date plasma emission code*
Free accessEDP Sciences | 2009|Keywords: ISM: evolution -
Chemical Evolution During the Formation of Molecular Clouds
IOP Institute of Physics | 2022|Keywords: (ISM:) evolution -
Phenol in High-mass Star-forming Regions
IOP Institute of Physics | 2022|Keywords: (ISM:) evolution -
Spatially resolved signature of quenching in star-forming galaxies
Free accessBASE | 2019|Keywords: ISM: evolution -
The N2D+/N2H+ ratio as an evolutionary tracer of Class 0 protostars*
Free accessEDP Sciences | 2009|Keywords: ISM: evolution -
Revisiting the dust destruction efficiency of supernovae
Free accessBASE | 2020|Keywords: ISM: evolution -
Properties of shocked dust grains in supernova remnants
Free accessBASE | 2022|Keywords: ISM: evolution -
A simple and general method for solving detailed chemical evolution with delayed production of iron and other chemical elements
Free accessBASE | 2017|Keywords: ISM: evolution -
The spin temperature of high-redshift damped Lyman α systems
Free accessBASE | 2014|Keywords: ISM: evolution -
Gas-phase metallicity gradients of TNG50 star-forming galaxies
Free accessBASE | 2021|Keywords: ISM: evolution -
GGCHEMPY: A Pure Python-based Gas-grain Chemical Code for Efficient Simulation of Interstellar Chemistry*
Supported by CASSACA.
IOP Institute of Physics | 2022|Keywords: (ISM:) evolution -
GASTON: Galactic Star Formation with NIKA2-evidence for the mass growth of star-forming clumps
Free accessBASE | 2021|Keywords: ISM: evolution -
Metal abundances in the MACER simulations of the hot interstellar medium
Free accessBASE | 2020|Keywords: galaxies: active – galaxies: ISM – ISM: abundances – ISM: evolution -
Metal abundances in the MACER simulations of the hot interstellar medium
Wiley | 2020|Keywords: galaxies: active – galaxies: ISM – ISM: abundances – ISM: evolution -
MAMBO mapping of Spitzer c2d small clouds and cores ******
Free accessEDP Sciences | 2008|Keywords: ISM: evolution -
Artificial viscosity in simulation of shock waves by smoothed particle hydrodynamics
Online Contents | 2007|Keywords: ISM: evolution -
Chemical evolution during the process of proto-star formation by considering a two dimensional hydrodynamic model
Elsevier | 2013|Keywords: ISM: evolution
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