Submillimetre observations of the Z = 2.286 IRAS galaxy 10214 + 4724

D. L. Clements; M. Rowan-Robinson; A. Lawrence; T. Broadhurst

doi:10.1093/mnras/256.1.35P

Submillimetre observations of the Z = 2.286 IRAS galaxy 10214 + 4724

D. L. Clements, M. Rowan-Robinson, A. Lawrence, T. Broadhurst

School of Physics and Astronomy

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

Abstract

Results of submillimeter observations of the very high-redshift IRAS galaxy 10214 + 4724 are presented. Significant detections at 800 and 450 are achieved. The data are compared to the existing models of this galaxy, and it is found that both the extreme primeval galaxy model an the dust-embedded Seyfert model are excluded. The galaxy is likely to be undergoing and extreme starburst, but whether this represents the formation of a significant fraction of the stars is unclear.

Original language	English
Pages (from-to)	349
Journal	Monthly Notices of the Royal Astronomical Society
Volume	256
DOIs	https://doi.org/10.1093/mnras/256.1.35P
Publication status	Published - 1 May 1992

Keywords

Galactic Evolution
Galactic Radio Waves
Infrared Astronomy
Starburst Galaxies
Submillimeter Waves
Far Infrared Radiation
Infrared Astronomy Satellite
Red Shift

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title = "Submillimetre observations of the Z = 2.286 IRAS galaxy 10214 + 4724",

abstract = "Results of submillimeter observations of the very high-redshift IRAS galaxy 10214 + 4724 are presented. Significant detections at 800 and 450 are achieved. The data are compared to the existing models of this galaxy, and it is found that both the extreme primeval galaxy model an the dust-embedded Seyfert model are excluded. The galaxy is likely to be undergoing and extreme starburst, but whether this represents the formation of a significant fraction of the stars is unclear.",

keywords = "Galactic Evolution, Galactic Radio Waves, Infrared Astronomy, Starburst Galaxies, Submillimeter Waves, Far Infrared Radiation, Infrared Astronomy Satellite, Red Shift",

author = "Clements, {D. L.} and M. Rowan-Robinson and A. Lawrence and T. Broadhurst",

year = "1992",

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doi = "10.1093/mnras/256.1.35P",

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T1 - Submillimetre observations of the Z = 2.286 IRAS galaxy 10214 + 4724

AU - Clements, D. L.

AU - Rowan-Robinson, M.

AU - Lawrence, A.

AU - Broadhurst, T.

PY - 1992/5/1

Y1 - 1992/5/1

N2 - Results of submillimeter observations of the very high-redshift IRAS galaxy 10214 + 4724 are presented. Significant detections at 800 and 450 are achieved. The data are compared to the existing models of this galaxy, and it is found that both the extreme primeval galaxy model an the dust-embedded Seyfert model are excluded. The galaxy is likely to be undergoing and extreme starburst, but whether this represents the formation of a significant fraction of the stars is unclear.

AB - Results of submillimeter observations of the very high-redshift IRAS galaxy 10214 + 4724 are presented. Significant detections at 800 and 450 are achieved. The data are compared to the existing models of this galaxy, and it is found that both the extreme primeval galaxy model an the dust-embedded Seyfert model are excluded. The galaxy is likely to be undergoing and extreme starburst, but whether this represents the formation of a significant fraction of the stars is unclear.

KW - Galactic Evolution

KW - Galactic Radio Waves

KW - Infrared Astronomy

KW - Starburst Galaxies

KW - Submillimeter Waves

KW - Far Infrared Radiation

KW - Infrared Astronomy Satellite

KW - Red Shift

U2 - 10.1093/mnras/256.1.35P

DO - 10.1093/mnras/256.1.35P

M3 - Article

VL - 256

SP - 349

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

ER -