Extensive online shock model database

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Autore principale: A. Alarie
Natura: Artículo científico
Lingua:en
Pubblicazione: Universidad Nacional Autónoma de México 2019
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author A. Alarie
author_facet A. Alarie
contents Extensive online shock model database A. Alarie C. Morisset Física, Astronomía y Matemáticas ISM Galaxy abundances H II regions miscellaneous 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 interactively the database as it evolves with time. Examples of its usage are given using the Python language. 2019 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57171631021 https://www.redalyc.org/journal/571/57171631021/ https://www.redalyc.org/journal/571/57171631021/html/ https://www.redalyc.org/journal/571/57171631021/57171631021.epub https://www.redalyc.org/journal/571/57171631021/movil 10.22201/ia.01851101p.2019.55.02.21 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.55
format Artículo científico
id redalyc_57171631021
institution Redalyc
language en
publishDate 2019
publisher Universidad Nacional Autónoma de México
spellingShingle Extensive online shock model database
A. Alarie
Física, Astronomía y Matemáticas
ISM
Galaxy
abundances
H II regions
miscellaneous
Extensive online shock model database A. Alarie C. Morisset Física, Astronomía y Matemáticas ISM Galaxy abundances H II regions miscellaneous 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 interactively the database as it evolves with time. Examples of its usage are given using the Python language. 2019 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57171631021 https://www.redalyc.org/journal/571/57171631021/ https://www.redalyc.org/journal/571/57171631021/html/ https://www.redalyc.org/journal/571/57171631021/57171631021.epub https://www.redalyc.org/journal/571/57171631021/movil 10.22201/ia.01851101p.2019.55.02.21 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.55
title Extensive online shock model database
topic Física, Astronomía y Matemáticas
ISM
Galaxy
abundances
H II regions
miscellaneous
url https://www.redalyc.org/articulo.oa?id=57171631021
https://www.redalyc.org/journal/571/57171631021/
https://www.redalyc.org/journal/571/57171631021/html/
https://www.redalyc.org/journal/571/57171631021/57171631021.epub
https://www.redalyc.org/journal/571/57171631021/movil