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Extremely red compact radio sources - The empty field objectsRadiation of 10 microns has been detected from 1413+135, one of the very red objects discovered by Rieke, Lebofsky, and Kinman (1979) at near-infrared wavelengths. The spectrum of this object flattens at wavelengths longer than 2.2 microns. Upper limits are also given for the 10-micron emission from 2255+14, 0026+34, and 0406+121. Photometry between 1.25 and 2.2 microns confirms the variability of 1413+135, 2255+41, and 0406+121. Five percent resolution spectra of 1413+135 and 0406+121 between 1.5 and 2.4 microns show no emission or absorption lines. The spectral data rule out the possibility that 1413+135 is a quasar with normal line strengths and a redshift less than 1.3 and greater than 4. The lack of features of the 1.5-2.4-micron spectra, the rapid variability, and the overall shape of the radio, infrared, and X-ray energy distributions are consistent with a BL Lac nature for these objects.
Document ID
19810061576
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Beichman, C. A.
(California Inst. of Tech. Pasadena, CA, United States)
Neugebauer, G.
(California Inst. of Tech. Pasadena, CA, United States)
Soifer, B. T.
(California Inst. of Tech. Pasadena, CA, United States)
Matthews, K.
(Palomar Observatory Pasadena, CA, United States)
Wootten, H. A.
(California Institute of Technology; Owens Valley Radio Observatory Pasadena, CA, United States)
Pravdo, S. H.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 11, 2013
Publication Date
August 1, 1981
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
81A45980
Distribution Limits
Public
Copyright
Other

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