TY - JOUR
T1 - The near-infrared counterpart of a variable galactic plane radio source
AU - Margon, Bruce
AU - Phillips, Andrew C.
AU - Ciardullo, Robin
AU - Jacoby, George H.
N1 - Copyright:
Copyright 2018 Elsevier B.V., All rights reserved.
PY - 1992/3
Y1 - 1992/3
N2 - We have identified a near-infrared counterpart to the highly variable, unresolved galactic plane radio source GT 0116 + 622. This source is of particular interest, as it has been previously suggested to be the counterpart of the γ-ray source Cas γ-1. Our near-infrared and red images detect a faint, spatially extended (3″ FWHM), very red object coincident with the radio position. There is complex spatial structure which may be due in part to an unrelated superposed foreground object. Observations on multiple nights show no evidence for flux variability, despite the high amplitude variability on a timescale of days reported for the radio source. The data are consistent with an interpretation of GT 0116 + 622 as an unusually variable, obscured active galaxy at a distance of several hundred megaparsecs, although more exotic, and in particular galactic, interpretations cannot yet be ruled out. If the object is extragalactic, the previously suggested identification with the γ-ray source would seem unlikely.
AB - We have identified a near-infrared counterpart to the highly variable, unresolved galactic plane radio source GT 0116 + 622. This source is of particular interest, as it has been previously suggested to be the counterpart of the γ-ray source Cas γ-1. Our near-infrared and red images detect a faint, spatially extended (3″ FWHM), very red object coincident with the radio position. There is complex spatial structure which may be due in part to an unrelated superposed foreground object. Observations on multiple nights show no evidence for flux variability, despite the high amplitude variability on a timescale of days reported for the radio source. The data are consistent with an interpretation of GT 0116 + 622 as an unusually variable, obscured active galaxy at a distance of several hundred megaparsecs, although more exotic, and in particular galactic, interpretations cannot yet be ruled out. If the object is extragalactic, the previously suggested identification with the γ-ray source would seem unlikely.
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U2 - 10.1086/116113
DO - 10.1086/116113
M3 - Article
AN - SCOPUS:11944258770
SN - 0004-6256
VL - 103
SP - 924
EP - 926
JO - Astronomical Journal
JF - Astronomical Journal
IS - 3
ER -