The fingerprints of photoionization and shock-ionization in two CSS sources

We investigate the ionization state of the extended emission-line regions (EELRs) around two compact steep-spectrum (CSS) radio galaxies, 3C 268.3 and 3C 303.1, in order to identify the contribution of photoionization and shock-ionization. We perform a new spectroscopical (long-slit) analysis with G...

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Autores principales: Reynaldi, María Victoria, Feinstein Baigorri, Carlos
Formato: Articulo
Lenguaje:Inglés
Publicado: 2016
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93812
https://academic.oup.com/mnras/article-abstract/455/2/2242/1123596?redirectedFrom=fulltext
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id I19-R120-10915-93812
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Shock waves
Jets
Active galaxies
Outflows
Interstellar medium
3C 303.1 (galaxia)
3C 268.3 (galaxia)
spellingShingle Astronomía
Shock waves
Jets
Active galaxies
Outflows
Interstellar medium
3C 303.1 (galaxia)
3C 268.3 (galaxia)
Reynaldi, María Victoria
Feinstein Baigorri, Carlos
The fingerprints of photoionization and shock-ionization in two CSS sources
topic_facet Astronomía
Shock waves
Jets
Active galaxies
Outflows
Interstellar medium
3C 303.1 (galaxia)
3C 268.3 (galaxia)
description We investigate the ionization state of the extended emission-line regions (EELRs) around two compact steep-spectrum (CSS) radio galaxies, 3C 268.3 and 3C 303.1, in order to identify the contribution of photoionization and shock-ionization. We perform a new spectroscopical (long-slit) analysis with GMOS/Gemini with the slit oriented in the radio-jet direction, where outflows are known to exist. The [Ne V] λ3426 emission is the most interesting feature of the spectra and the one key to breaking the degeneracy between the models: since this emission-line is more extended than He II, it challenges the ionization structure proposed by any photoionization model, also its intensity relative to H β does not behave as expected with respect to the ionization parameter U in the same scenario. On the contrary, when it is compared to the intensity of [O II] λ3727/H β and all these results are joined, the whole scenario is plausible to be explained as emission coming from the hot, compressed, shocked gas in shock-ionization models. Although the model fitting is strongly sensitive to the chosen line ratios, it argues for the presence of external and strong ionizing fields, such as the precursor field created by the shock or/and the AGN radiation field. In this paper, we show how AGN photoionization and shock-ionization triggered by jet–cloud interaction work together in these EELRs in order to explain the observed trends and line-ratio behaviours in a kinematically acceptable way.
format Articulo
Articulo
author Reynaldi, María Victoria
Feinstein Baigorri, Carlos
author_facet Reynaldi, María Victoria
Feinstein Baigorri, Carlos
author_sort Reynaldi, María Victoria
title The fingerprints of photoionization and shock-ionization in two CSS sources
title_short The fingerprints of photoionization and shock-ionization in two CSS sources
title_full The fingerprints of photoionization and shock-ionization in two CSS sources
title_fullStr The fingerprints of photoionization and shock-ionization in two CSS sources
title_full_unstemmed The fingerprints of photoionization and shock-ionization in two CSS sources
title_sort fingerprints of photoionization and shock-ionization in two css sources
publishDate 2016
url http://sedici.unlp.edu.ar/handle/10915/93812
https://academic.oup.com/mnras/article-abstract/455/2/2242/1123596?redirectedFrom=fulltext
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