Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.

We present long-slit spectroscopy and imaging data obtained with the Focal Reducer and Low Dispersion Spectrograph (FORS2) on the Very Large Telescope of 13 optically selected type 2 quasars at z ∼ 0.3–0.6 from the original sample of Zakamska et al. (2003). The sample is likely to be affected by dif...

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Detalles Bibliográficos
Autor: Andrew Humphrey
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2011
País:México
Institución:Instituto Nacional de Astrofísica, Óptica y Electrónica
Repositorio:Repositorio Institucional del INAOE
Idioma:inglés
OAI Identifier:oai:inaoe.repositorioinstitucional.mx:1009/1885
Acceso en línea:http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1885
Access Level:acceso abierto
Palabra clave:info:eu-repo/classification/Inspec/Galaxies: active
info:eu-repo/classification/Inspec/Quasars: emission lines
info:eu-repo/classification/Inspec/Quasars: general
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
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spelling Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.Andrew Humphreyinfo:eu-repo/classification/Inspec/Galaxies: activeinfo:eu-repo/classification/Inspec/Quasars: emission linesinfo:eu-repo/classification/Inspec/Quasars: generalinfo:eu-repo/classification/cti/1info:eu-repo/classification/cti/21info:eu-repo/classification/cti/21We present long-slit spectroscopy and imaging data obtained with the Focal Reducer and Low Dispersion Spectrograph (FORS2) on the Very Large Telescope of 13 optically selected type 2 quasars at z ∼ 0.3–0.6 from the original sample of Zakamska et al. (2003). The sample is likely to be affected by different selection biases.We investigate the evidence for (i) mergers/interactions (ii) star formation activity in the neighbourhood of the quasars and (iii) extended emission-line regions (EELRs) and their nature. Evidence for mergers/interactions is found in 5/13 objects. This is a lower limit for our sample, given the shallowness ofmost of our continuum images. Although active galactic nucleus (AGN) photoionization cannot be totally discarded, line ratios consistent with stellar photoionization are found in general in companion galaxies/knots/nuclei near these same objects. On the contrary, the gas in the neighbourhood of the quasar nucleus shows line ratios inconsistent with HII galaxies and typical of AGN photoionized nebulae. A natural scenario to explain the observations is that star formation is ongoing in companion galaxies/knots/nuclei, possibly triggered by the interactions. These systems are, therefore, composite in their emission-line properties showing a combination of AGN and star formation features. EELRs have been found in 7/13 objects, although this fraction might be higher if a complete spatial coverage around the quasars was performed. The sizes vary between a few and up to 64 kpc. In general, the EELR apparently consists of an extended nebula associated with the quasar. In at least one case, the EELR is associated with ionized tidal features.Monthly Notices of the Royal Astronomical Society2011info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1885reponame:Repositorio Institucional del INAOEinstname:Instituto Nacional de Astrofísica, Óptica y Electrónicainstacron:INAOEengcitation:Villar Martín, M., et al., (2011), Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6. , Monthly Notices of the Royal Astronomical Society, Vol. 416(1): 262–278info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0oai:inaoe.repositorioinstitucional.mx:1009/18852024-08-28T03:23:01Z
dc.title.none.fl_str_mv Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
title Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
spellingShingle Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
Andrew Humphrey
info:eu-repo/classification/Inspec/Galaxies: active
info:eu-repo/classification/Inspec/Quasars: emission lines
info:eu-repo/classification/Inspec/Quasars: general
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
title_short Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
title_full Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
title_fullStr Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
title_full_unstemmed Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
title_sort Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6.
dc.creator.none.fl_str_mv Andrew Humphrey
author Andrew Humphrey
author_facet Andrew Humphrey
author_role author
dc.subject.none.fl_str_mv info:eu-repo/classification/Inspec/Galaxies: active
info:eu-repo/classification/Inspec/Quasars: emission lines
info:eu-repo/classification/Inspec/Quasars: general
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
topic info:eu-repo/classification/Inspec/Galaxies: active
info:eu-repo/classification/Inspec/Quasars: emission lines
info:eu-repo/classification/Inspec/Quasars: general
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
description We present long-slit spectroscopy and imaging data obtained with the Focal Reducer and Low Dispersion Spectrograph (FORS2) on the Very Large Telescope of 13 optically selected type 2 quasars at z ∼ 0.3–0.6 from the original sample of Zakamska et al. (2003). The sample is likely to be affected by different selection biases.We investigate the evidence for (i) mergers/interactions (ii) star formation activity in the neighbourhood of the quasars and (iii) extended emission-line regions (EELRs) and their nature. Evidence for mergers/interactions is found in 5/13 objects. This is a lower limit for our sample, given the shallowness ofmost of our continuum images. Although active galactic nucleus (AGN) photoionization cannot be totally discarded, line ratios consistent with stellar photoionization are found in general in companion galaxies/knots/nuclei near these same objects. On the contrary, the gas in the neighbourhood of the quasar nucleus shows line ratios inconsistent with HII galaxies and typical of AGN photoionized nebulae. A natural scenario to explain the observations is that star formation is ongoing in companion galaxies/knots/nuclei, possibly triggered by the interactions. These systems are, therefore, composite in their emission-line properties showing a combination of AGN and star formation features. EELRs have been found in 7/13 objects, although this fraction might be higher if a complete spatial coverage around the quasars was performed. The sizes vary between a few and up to 64 kpc. In general, the EELR apparently consists of an extended nebula associated with the quasar. In at least one case, the EELR is associated with ionized tidal features.
publishDate 2011
dc.date.none.fl_str_mv 2011
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/acceptedVersion
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1885
url http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1885
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv citation:Villar Martín, M., et al., (2011), Interactions, star formation and extended nebulae in SDSS type 2 quasars at 0.3 ≲ z ≲ 0.6. , Monthly Notices of the Royal Astronomical Society, Vol. 416(1): 262–278
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-nd/4.0
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-nd/4.0
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
publisher.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
dc.source.none.fl_str_mv reponame:Repositorio Institucional del INAOE
instname:Instituto Nacional de Astrofísica, Óptica y Electrónica
instacron:INAOE
instname_str Instituto Nacional de Astrofísica, Óptica y Electrónica
instacron_str INAOE
institution INAOE
reponame_str Repositorio Institucional del INAOE
collection Repositorio Institucional del INAOE
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repository.mail.fl_str_mv
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