EXTENSIVE ONLINE SHOCK MODEL DATABASE

@article{Alarie2019EXTENSIVEOS,
  title={EXTENSIVE ONLINE SHOCK MODEL DATABASE},
  author={Alexandre Alarie and Christophe Morisset},
  journal={Revista Mexicana de Astronom{\'i}a y Astrof{\'i}sica},
  year={2019}
}
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

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References

SHOWING 1-10 OF 18 REFERENCES
The MAPPINGS III Library of Fast Radiative Shock Models
We present a new library of fully-radiative shock models calculated with the MAPPINGS III shock and photoionization code. The library consists of grids of models with shock velocities in the rangeExpand
Ultraviolet observations of the Cygnus Loop
The analysis of IUE observations of a filament on the western edge of the Cygnus Loop yields a shock velocity of about 130 km/sec, significantly higher than the velocity estimated from the opticalExpand
Effects of Preionization in Radiative Shocks. I. Self-consistent Models
In this paper we treat the pre-ionisation problem in shocks over the velocity range $10 < v_{\rm s} < 1500$\,km/s in a self-consistent manner. We identify four distinct classes of solution controlledExpand
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
In this paper, we combine the stellar spectral synthesis code STARBURST99, the nebular modeling code MAPPINGS IIIq, a one-dimensional dynamical evolution model of H ii regions around massive clustersExpand
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
An investigation is made of the merits of various emission-line intensity ratios for classifying the spectra of extragalactic objects. It is shown empirically that several combinations ofExpand
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
We have modeled a large sample of infrared starburst galaxies using both the PEGASE v2.0 and STARBURST99 codes to generate the spectral energy distribution (SED) of the young star clusters. PEGASEExpand
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