The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724

M. Rowan-Robinson; A. Efstathiou; A. Lawrence; S. Oliver; A. Taylor; T. J. Broadhurst; R. G. McMahon; C. R. Benn; J. J. Condon; C. J. Lonsdale; P. Hacking; T. Conrow; W. S. Saunders; D. L. Clements; R. S. Ellis; I. Robson

doi:10.1093/mnras/261.3.513

The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724

M. Rowan-Robinson, A. Efstathiou, A. Lawrence, S. Oliver, A. Taylor, T. J. Broadhurst, R. G. McMahon, C. R. Benn, J. J. Condon, C. J. Lonsdale, P. Hacking, T. Conrow, W. S. Saunders, D. L. Clements, R. S. Ellis, I. Robson

School of Physics and Astronomy

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

Abstract

New observations and theoretical models for the continuous UV-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F10214 + 4724 are presented. The radio spectrum at 1.49-8.44 GHz and the resolved nature of the radio source are compatible with a synchrotron origin of the radio radiation associated with a luminous starburst. The submillimeter and FIR spectrum is modeled in terms of emission from both spherically symmetric dust clouds and an axially symmetric flared disk. The observed optical to near-IR continuum derived from WHT-FOS spectroscopy and from UKIRT observations is interpreted in terms of reddened QSO and starburst models. The continuum is broadly consistent with emission from a QSO reddened by 1.5 mag of dust. The radio, submillimeter, FIR, and CO observations of IRAS F10214 + 4724 are consistent with a powerful starburst early in the life of a massive galaxy.

Original language	English
Pages (from-to)	513-521
Journal	Monthly Notices of the Royal Astronomical Society
Volume	261
DOIs	https://doi.org/10.1093/mnras/261.3.513
Publication status	Published - 1 Apr 1993

Keywords / Materials (for Non-textual outputs)

Continuous Radiation
Infrared Astronomy Satellite
Radio Emission
Ultraviolet Astronomy
Astronomical Models
Radio Astronomy

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10.1093/mnras/261.3.513

http://adsabs.harvard.edu/abs/1993MNRAS.261..513R

Cite this

Rowan-Robinson, M., Efstathiou, A., Lawrence, A., Oliver, S., Taylor, A., Broadhurst, T. J., McMahon, R. G., Benn, C. R., Condon, J. J., Lonsdale, C. J., Hacking, P., Conrow, T., Saunders, W. S., Clements, D. L., Ellis, R. S., & Robson, I. (1993). The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724. Monthly Notices of the Royal Astronomical Society, 261, 513-521. https://doi.org/10.1093/mnras/261.3.513

@article{65a227eac7b2438b90a8384517a85130,

title = "The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724",

abstract = "New observations and theoretical models for the continuous UV-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F10214 + 4724 are presented. The radio spectrum at 1.49-8.44 GHz and the resolved nature of the radio source are compatible with a synchrotron origin of the radio radiation associated with a luminous starburst. The submillimeter and FIR spectrum is modeled in terms of emission from both spherically symmetric dust clouds and an axially symmetric flared disk. The observed optical to near-IR continuum derived from WHT-FOS spectroscopy and from UKIRT observations is interpreted in terms of reddened QSO and starburst models. The continuum is broadly consistent with emission from a QSO reddened by 1.5 mag of dust. The radio, submillimeter, FIR, and CO observations of IRAS F10214 + 4724 are consistent with a powerful starburst early in the life of a massive galaxy.",

keywords = "Continuous Radiation, Infrared Astronomy Satellite, Radio Emission, Ultraviolet Astronomy, Astronomical Models, Radio Astronomy",

author = "M. Rowan-Robinson and A. Efstathiou and A. Lawrence and S. Oliver and A. Taylor and Broadhurst, {T. J.} and McMahon, {R. G.} and Benn, {C. R.} and Condon, {J. J.} and Lonsdale, {C. J.} and P. Hacking and T. Conrow and Saunders, {W. S.} and Clements, {D. L.} and Ellis, {R. S.} and I. Robson",

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month = apr,

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doi = "10.1093/mnras/261.3.513",

language = "English",

volume = "261",

pages = "513--521",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

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Rowan-Robinson, M, Efstathiou, A, Lawrence, A, Oliver, S, Taylor, A, Broadhurst, TJ, McMahon, RG, Benn, CR, Condon, JJ, Lonsdale, CJ, Hacking, P, Conrow, T, Saunders, WS, Clements, DL, Ellis, RS & Robson, I 1993, 'The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724', Monthly Notices of the Royal Astronomical Society, vol. 261, pp. 513-521. https://doi.org/10.1093/mnras/261.3.513

TY - JOUR

T1 - The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724

AU - Rowan-Robinson, M.

AU - Efstathiou, A.

AU - Lawrence, A.

AU - Oliver, S.

AU - Taylor, A.

AU - Broadhurst, T. J.

AU - McMahon, R. G.

AU - Benn, C. R.

AU - Condon, J. J.

AU - Lonsdale, C. J.

AU - Hacking, P.

AU - Conrow, T.

AU - Saunders, W. S.

AU - Clements, D. L.

AU - Ellis, R. S.

AU - Robson, I.

PY - 1993/4/1

Y1 - 1993/4/1

N2 - New observations and theoretical models for the continuous UV-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F10214 + 4724 are presented. The radio spectrum at 1.49-8.44 GHz and the resolved nature of the radio source are compatible with a synchrotron origin of the radio radiation associated with a luminous starburst. The submillimeter and FIR spectrum is modeled in terms of emission from both spherically symmetric dust clouds and an axially symmetric flared disk. The observed optical to near-IR continuum derived from WHT-FOS spectroscopy and from UKIRT observations is interpreted in terms of reddened QSO and starburst models. The continuum is broadly consistent with emission from a QSO reddened by 1.5 mag of dust. The radio, submillimeter, FIR, and CO observations of IRAS F10214 + 4724 are consistent with a powerful starburst early in the life of a massive galaxy.

AB - New observations and theoretical models for the continuous UV-to-radio spectrum of the ultraluminous protogalaxy candidate IRAS F10214 + 4724 are presented. The radio spectrum at 1.49-8.44 GHz and the resolved nature of the radio source are compatible with a synchrotron origin of the radio radiation associated with a luminous starburst. The submillimeter and FIR spectrum is modeled in terms of emission from both spherically symmetric dust clouds and an axially symmetric flared disk. The observed optical to near-IR continuum derived from WHT-FOS spectroscopy and from UKIRT observations is interpreted in terms of reddened QSO and starburst models. The continuum is broadly consistent with emission from a QSO reddened by 1.5 mag of dust. The radio, submillimeter, FIR, and CO observations of IRAS F10214 + 4724 are consistent with a powerful starburst early in the life of a massive galaxy.

KW - Continuous Radiation

KW - Infrared Astronomy Satellite

KW - Radio Emission

KW - Ultraviolet Astronomy

KW - Astronomical Models

KW - Radio Astronomy

U2 - 10.1093/mnras/261.3.513

DO - 10.1093/mnras/261.3.513

M3 - Article

SN - 0035-8711

VL - 261

SP - 513

EP - 521

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

ER -

The ultraviolet-to-radio continuum of the ultraluminous galaxy IRAS F10214 + 4724

Abstract

Keywords / Materials (for Non-textual outputs)

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