The pan-spectral energy distribution of dusty narrow line regions

Brent A. Groves; Michael A. Dopita; Ralph S. Sutherland

doi:10.1063/1.1913939

The pan-spectral energy distribution of dusty narrow line regions

Brent A. Groves^*, Michael A. Dopita, Ralph S. Sutherland

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › peer-review

1 Citation (Scopus)

Abstract

Narrow line regions (NLR) are a major component of active galaxies, and commonly used as an indicator of the presence of an active galactic nucleus (AGN). Most of the analysis and theoretical work into NLRs so far has concentrated only on the narrow emission lines. However, NLRs show strong evidence of containing dust and will likely emit strongly in the infrared. Here, we model this radiation from NLRs, examining the effects of pressure and ionization parameter, and demonstrate that a large fraction of the NLR emission is emerges in the IR.

Original language	English
Title of host publication	SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES
Subtitle of host publication	Confronting Models with Data - International Workshop
Pages	273-276
Number of pages	4
DOIs	https://doi.org/10.1063/1.1913939
Publication status	Published - 11 Apr 2005
Event	SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop - Heidelberg, Germany Duration: 4 Oct 2004 → 8 Oct 2004

Publication series

Name	AIP Conference Proceedings
Volume	761
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop
Country/Territory	Germany
City	Heidelberg
Period	4/10/04 → 8/10/04

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10.1063/1.1913939

Cite this

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title = "The pan-spectral energy distribution of dusty narrow line regions",

abstract = "Narrow line regions (NLR) are a major component of active galaxies, and commonly used as an indicator of the presence of an active galactic nucleus (AGN). Most of the analysis and theoretical work into NLRs so far has concentrated only on the narrow emission lines. However, NLRs show strong evidence of containing dust and will likely emit strongly in the infrared. Here, we model this radiation from NLRs, examining the effects of pressure and ionization parameter, and demonstrate that a large fraction of the NLR emission is emerges in the IR.",

author = "Groves, \{Brent A.\} and Dopita, \{Michael A.\} and Sutherland, \{Ralph S.\}",

year = "2005",

month = apr,

day = "11",

doi = "10.1063/1.1913939",

language = "English",

isbn = "0735402469",

series = "AIP Conference Proceedings",

pages = "273--276",

booktitle = "SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES",

note = "SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop ; Conference date: 04-10-2004 Through 08-10-2004",

}

Groves, BA, Dopita, MA & Sutherland, RS 2005, The pan-spectral energy distribution of dusty narrow line regions. in SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop. AIP Conference Proceedings, vol. 761, pp. 273-276, SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop, Heidelberg, Germany, 4/10/04. https://doi.org/10.1063/1.1913939

The pan-spectral energy distribution of dusty narrow line regions. / Groves, Brent A.; Dopita, Michael A.; Sutherland, Ralph S.
SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop. 2005. p. 273-276 (AIP Conference Proceedings; Vol. 761).

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › peer-review

TY - GEN

T1 - The pan-spectral energy distribution of dusty narrow line regions

AU - Groves, Brent A.

AU - Dopita, Michael A.

AU - Sutherland, Ralph S.

PY - 2005/4/11

Y1 - 2005/4/11

N2 - Narrow line regions (NLR) are a major component of active galaxies, and commonly used as an indicator of the presence of an active galactic nucleus (AGN). Most of the analysis and theoretical work into NLRs so far has concentrated only on the narrow emission lines. However, NLRs show strong evidence of containing dust and will likely emit strongly in the infrared. Here, we model this radiation from NLRs, examining the effects of pressure and ionization parameter, and demonstrate that a large fraction of the NLR emission is emerges in the IR.

AB - Narrow line regions (NLR) are a major component of active galaxies, and commonly used as an indicator of the presence of an active galactic nucleus (AGN). Most of the analysis and theoretical work into NLRs so far has concentrated only on the narrow emission lines. However, NLRs show strong evidence of containing dust and will likely emit strongly in the infrared. Here, we model this radiation from NLRs, examining the effects of pressure and ionization parameter, and demonstrate that a large fraction of the NLR emission is emerges in the IR.

UR - https://www.scopus.com/pages/publications/33645295571

U2 - 10.1063/1.1913939

DO - 10.1063/1.1913939

M3 - Conference Paper

SN - 0735402469

SN - 9780735402461

T3 - AIP Conference Proceedings

SP - 273

EP - 276

BT - SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES

T2 - SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data - International Workshop

Y2 - 4 October 2004 through 8 October 2004

ER -

The pan-spectral energy distribution of dusty narrow line regions

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