The 0.3 to 100 Micron Continua

M. J. Ward; N. P. Carleton; M. Elvis; G. Fabbiano; S. P. Willner; A. Lawrence

The 0.3 to 100 Micron Continua

M. J. Ward, N. P. Carleton, M. Elvis, G. Fabbiano, S. P. Willner, A. Lawrence

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

The continua of type 1 Seyferts from 0.3 to 100 microns have been examined. The authors focus on the modifying effects of dust, both in terms of absorption and re-radiation. After allowance is made for dust and the presence of extranuclear contributions to the IRAS fluxes, there remains a ubiquitous underlying distribution which the authors believe to be non-thermal. There is evidence that the thermal infrared components corresponding to hot and warm dust may be associated with the broad and narrow emission line regions.

Original language	English
Title of host publication	Observational Evidence of Activity in Galaxies: Proceedings of the 121st Symposium of the International Astronomical Union
Pages	119
Volume	121
Publication status	Published - 31 Dec 1986

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@inproceedings{c0d697a4cb674b1a998f1261ec0a304a,

title = "The 0.3 to 100 Micron Continua",

abstract = "The continua of type 1 Seyferts from 0.3 to 100 microns have been examined. The authors focus on the modifying effects of dust, both in terms of absorption and re-radiation. After allowance is made for dust and the presence of extranuclear contributions to the IRAS fluxes, there remains a ubiquitous underlying distribution which the authors believe to be non-thermal. There is evidence that the thermal infrared components corresponding to hot and warm dust may be associated with the broad and narrow emission line regions.",

author = "Ward, \{M. J.\} and Carleton, \{N. P.\} and M. Elvis and G. Fabbiano and Willner, \{S. P.\} and A. Lawrence",

note = "Observational Evidence of Activity in Galaxies: Proceedings of the 121st Symposium of the International Astronomical Union, held in Byurakan, Armenia, U.S.S.R., June 3-7, 1986. Edited by E. E. Khachikian, Klaus J. Fricke and Jorge Melnick. International Astronomical Union. Symposium no. 121, Kluwer Academic Publishers, Dordrecht",

year = "1986",

month = dec,

day = "31",

language = "English",

volume = "121",

pages = "119",

booktitle = "Observational Evidence of Activity in Galaxies: Proceedings of the 121st Symposium of the International Astronomical Union",

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TY - GEN

T1 - The 0.3 to 100 Micron Continua

AU - Ward, M. J.

AU - Carleton, N. P.

AU - Elvis, M.

AU - Fabbiano, G.

AU - Willner, S. P.

AU - Lawrence, A.

N1 - Observational Evidence of Activity in Galaxies: Proceedings of the 121st Symposium of the International Astronomical Union, held in Byurakan, Armenia, U.S.S.R., June 3-7, 1986. Edited by E. E. Khachikian, Klaus J. Fricke and Jorge Melnick. International Astronomical Union. Symposium no. 121, Kluwer Academic Publishers, Dordrecht

PY - 1986/12/31

Y1 - 1986/12/31

N2 - The continua of type 1 Seyferts from 0.3 to 100 microns have been examined. The authors focus on the modifying effects of dust, both in terms of absorption and re-radiation. After allowance is made for dust and the presence of extranuclear contributions to the IRAS fluxes, there remains a ubiquitous underlying distribution which the authors believe to be non-thermal. There is evidence that the thermal infrared components corresponding to hot and warm dust may be associated with the broad and narrow emission line regions.

AB - The continua of type 1 Seyferts from 0.3 to 100 microns have been examined. The authors focus on the modifying effects of dust, both in terms of absorption and re-radiation. After allowance is made for dust and the presence of extranuclear contributions to the IRAS fluxes, there remains a ubiquitous underlying distribution which the authors believe to be non-thermal. There is evidence that the thermal infrared components corresponding to hot and warm dust may be associated with the broad and narrow emission line regions.

M3 - Conference contribution

VL - 121

SP - 119

BT - Observational Evidence of Activity in Galaxies: Proceedings of the 121st Symposium of the International Astronomical Union

ER -

The 0.3 to 100 Micron Continua

Abstract

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