Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 50m 17.47943s |
Declination | +07° 54′ 08.6934″ |
Apparent magnitude (V) | 6.484 |
Characteristics | |
Spectral type | B2.5IVe |
U−B color index | -0.7 |
B−V color index | -0.1 |
Variable type | Be star |
Astrometry | |
Radial velocity (Rv) | -30.10 ± 5 km/s |
Proper motion (μ) | RA: -0.77 ± 0.39 mas/yr Dec.: -5.44 ± 0.46 mas/yr |
Parallax (π) | 1.89 ± 0.45 mas |
Distance | approx. 1,700 ly (approx. 500 pc) |
Details | |
Mass | 13.0[2] M☉ |
Radius | 7.7[2] R☉ |
Temperature | 23310[2] K |
Other designations | |
Database references | |
SIMBAD | data |
V1339 Aquilae, also known as HD 187567, is a Be star in the constellation Aquila. At its brightest its apparent magnitude is 6.22,[3] making it barely visible to the naked eye at a location with very little light pollution. It is located just 8 arc seconds from the center of the open cluster NGC 6828.[4]
V1339 Aquilae was discovered to be a Be star in 1925 by P. W. Merrill, M. L. Humason and C. G. Burwell.[5] The star's variability was detected in 1966 by A. W. J. Cousins, R. Lake and R. H. Stoy,[6] and because of this it was given its variable star designation, V1339 Aquilae, in 1979.[7]
V1339 Aquilae is around 13 times as massive as the Sun and has 7.7 times its diameter.[2] Its binary nature was discovered by speckle interferometry in 1983, at the Kitt Peak 4 meter telescope. At the time of these speckle observations the stars were separated by 0.057 arc seconds.[8]
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