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From: IAUC mailing list
Subject: IAUC 7086: 1999B; 1999A; V1333 Aql

Circular No. 7086
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
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V1333 AQUILAE
P. J. Callanan, University College, Cork; A. V. Filippenko,
University of California at Berkeley; and M. R. Garcia, Harvard-
Smithsonian Center for Astrophysics, write: "We imaged the
transient low-mass x-ray binary Aql X-1 = V1333 Aql with the Near
Infrared Camera on Keck I on 1998 Sept. 29.30 UT, while Aql X-1 was
in quiescence according to XTE ASM observations. Our K-band images
clearly resolve V1333 Aql into two stars, with a separation of 0".46.
The stars lie approximately along the east-west direction, with the
easterly star contributing 60 percent of the combined flux at K.
Z-band (about 1.05-micron) observations indicate that this star is
also somewhat bluer than its neighbor, and we speculate that this
may be the true infrared/optical counterpart of Aql X-1. Further
analysis is in progress to constrain the contamination of the V1333
Aql optical flux due to the line-of-sight interloper."

(C) Copyright 1999 CBAT
1999 January 15 (7086) Daniel W. E. Green