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Unidentified IRAS sources: Ultrahigh luminosity galaxiesOptical imaging and spectroscopy measurements were obtained for six of the high galactic latitude infrared sources reported by Houck, et al. (1984) from the IRAS survey to have no obvious optical counterparts on the POSS prints. All are identified with visually faint galaxies that have total luminosities in the range 5 x 10 to the 11th power stellar luminosity to 5 x 10 to the 12th power stellar luminosity. This luminosity emerges virtually entirely in the infrared. The origin of the luminosity, which is one to two orders of magnitude greater than that of normal galaxies, is not known at this time.
Document ID
19850007228
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Houck, J. R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Schneider, D. P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Danielson, G. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Beichman, C. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lonsdale, C. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Neugebauer, G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Soifer, B. T.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1985
Subject Category
Astronomy
Report/Patent Number
NAS 1.26:174207
NASA-CR-174207
Accession Number
85N15537
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-14134
CONTRACT_GRANT: NSF AST-83-12699
CONTRACT_GRANT: NAS5-25451
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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