AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

M. A. Dopita; M. Reuland; B. Groves; H. Röttgering; W. Van Breugel

doi:10.1002/asna.200510498

AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

M. A. Dopita^*, M. Reuland, B. Groves, H. Röttgering, W. Van Breugel

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

1 Citation (Scopus)

Abstract

Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due to an embedded AGN and is determining the attenuation of the galaxian light due to foreground dust.

Original language	English
Pages (from-to)	155-158
Number of pages	4
Journal	Astronomische Nachrichten
Volume	327
Issue number	2-3
DOIs	https://doi.org/10.1002/asna.200510498
Publication status	Published - 2006

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10.1002/asna.200510498

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title = "AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies",

abstract = "Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due to an embedded AGN and is determining the attenuation of the galaxian light due to foreground dust.",

keywords = "Galaxies: high redshift, Galaxies: star formation, Interstellar medium: galaxies",

author = "Dopita, \{M. A.\} and M. Reuland and B. Groves and H. R{\"o}ttgering and \{Van Breugel\}, W.",

year = "2006",

doi = "10.1002/asna.200510498",

language = "English",

volume = "327",

pages = "155--158",

journal = "Astronomische Nachrichten",

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T1 - AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

AU - Dopita, M. A.

AU - Reuland, M.

AU - Groves, B.

AU - Röttgering, H.

AU - Van Breugel, W.

PY - 2006

Y1 - 2006

N2 - Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due to an embedded AGN and is determining the attenuation of the galaxian light due to foreground dust.

AB - Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due to an embedded AGN and is determining the attenuation of the galaxian light due to foreground dust.

KW - Galaxies: high redshift

KW - Galaxies: star formation

KW - Interstellar medium: galaxies

UR - https://www.scopus.com/pages/publications/33645309871

U2 - 10.1002/asna.200510498

DO - 10.1002/asna.200510498

M3 - Article

SN - 0004-6337

VL - 327

SP - 155

EP - 158

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

IS - 2-3

ER -

AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

Abstract

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