A&A 367, 250-252 (2001)
DOI: 10.1051/0004-6361:20000457
Infrared photometry of the final flash star V605 Aquilae
K. H. Hinkle, R. R. Joyce and A. HeddenNational Optical Astronomy Observatory (Operated by the Association of Universities for Research in Astronomy, Inc. under cooperative agreement with the National Science Foundation.) , 950 N. Cherry Avenue, PO Box 26732, Tucson, 85726, USA
(Received 4 September 2000 / Accepted 24 November 2000 )
Abstract
We have obtained
infrared images in the J, H, and K bands of the field
containing
the post-AGB final-flash object V605 Aql. V605 Aql is the central
star of the planetary nebula A58 but has been incorrectly identified
with other stars in this field. In the infrared images V605 Aql appears as
a very red star at the position of the A58 center.
We present JHK photometry on two dates as well as astrometry of
V605 Aql. The infrared light from V605 Aql
originates in a thick dust cloud surrounding the star. There
is no indication of variability over a three month time period.
Key words: stars: evolution -- stars: individual: V605 Aql -- stars: AGB and post-AGB -- planetary nebulae: individual: A58 -- infrared: stars
Offprint request: K. H. Hinkle, hinkle@noao.edu
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