author={Alexandre Alarie and Christophe Morisset},
  journal={Revista Mexicana de Astronom{\'i}a y Astrof{\'i}sica},
We present a new database of fully radiative shock models calculated with the shock and photoionization code mappings v. The database architecture is built to contain diverse shock grids comprising of multiple shock parameters. It can be easily accessible through the MySQL protocol. Intensities of spectral lines from infrared to X-rays are stored along with other useful outputs such as the ionic fractions/temperature, integrated densities, etc. A web page was created in order to explore… Expand

Paper Mentions

Chemical abundances of Seyfert 2 AGNs – IV. Composite models calculated by photoionization + shocks
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Star formation in the nearby dwarf galaxy DDO 53: interplay between gas accretion and stellar feedback
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H ii regions in the CALIFA survey: I. catalogue presentation
We thank the referee for the helpful comments that have improved the quality of this article. We are grateful for the support of CONACYT grants CB-285080, FC-2016-01-1916, and CB2015-254132, andExpand
MUSE view of Arp220: Kpc-scale multi-phase outflow and evidence for positive feedback
Arp220 is the nearest and prototypical ULIRG, and shows evidence of pc-scale molecular outflows in its nuclear regions and strongly perturbed ionised gas kinematics on kpc scales. It is therefore theExpand
WARPFIELD-EMP: The self-consistent prediction of emission lines from evolving H ii regions in dense molecular clouds
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The MAPPINGS III Library of Fast Radiative Shock Models
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Ultraviolet observations of the Cygnus Loop
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Effects of Preionization in Radiative Shocks. I. Self-consistent Models
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Ultraviolet spectra of the Cygnus loop-depletion of the heavy elements
A comparison between the observed UV spectra and detailed consistent calculations of the Cygnus Loop is presented. The results demonstrate that the spectra can be explained by supposing that theExpand
Modeling the Pan-Spectral Energy Distribution of Starburst Galaxies. I. The Role of ISM Pressure and the Molecular Cloud Dissipation Timescale
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The Shocking Power Sources of LINERs
The majority of low-ionization nuclear emission-line regions (LINERs) harbor supermassive black holes with very low accretion rates. However, the accretion flows do not produce enough ionizingExpand
Spatial and spectral interpretation of a bright filament in the Cygnus Loop
A comparison is made of optical and UV line intensities and spatial and spectral optical line profiles of a well-defined Cygnus Loop filament with theoretical models. It is found that the sharpExpand
Classification parameters for the emission-line spectra of extragalactic objects
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Abundances of the heavy elements in the Magellanic Clouds. III - Interpretation of results
Chemical and structural evolutionary models for the Magellanic Clouds assuming bimodal star formation and gas infall are presented. The models are discussed in relation to the observed chemicalExpand
Theoretical Modeling of Starburst Galaxies
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