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HD 187279


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Study of the IR-excess supergiant HD 331319
We report the discovery of brightness variability in the IR-excess earlyF supergiant HD 331319, a candidate post-AGB star. Over three years ofsystematic U BV observations, the star showed low-amplitude (up to in V)quasi-periodic brightness variations on a time scale of ˜45 days. Apreliminary analysis of our photometry indicates that HD 331319 andother typical post-AGBF supergiants have a similar pattern ofvariability. A study of the extinction toward HD 331319 leads us toconclude that the fraction of the circumstellar extinction is small forthis star. We present low-resolution spectroscopy for HD 331319 anddiscuss the spectral classification of post-AGB F supergiants using HD331319, HD 161796, HD 187885, and HD 56126 as examples.

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UvbyHbeta_ photometry of main sequence A type stars.
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Observation and Astrometry data

Constellation:Cygne
Right ascension:19h47m59.64s
Declination:+31°30'22.6"
Apparent magnitude:6.798
Distance:91.408 parsecs
Proper motion RA:7
Proper motion Dec:14.1
B-T magnitude:6.935
V-T magnitude:6.81

Catalogs and designations:
Proper Names
HD 1989HD 187279
TYCHO-2 2000TYC 2656-5242-1
USNO-A2.0USNO-A2 1200-13261735
HIPHIP 97416

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