FG Virginis

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FG Virginis

Visual band light curves for FG Virginis, adapted from Breger et al. (1995)[1]
Observation data
J2000.0
Constellation Virgo
Right ascension 12h 14m 15.457s[2]
Declination −05° 42′ 59.75″[2]
Apparent magnitude (V) 6.56[3] (6.53 to 6.58)[4]
Characteristics
Evolutionary stage Main sequence
Spectral type A8/9V[5]
U−B color index 0.05[6]
B−V color index 0.277±0.007[3]
Variable type δ Sct[4]
Distance
273.5 ± 0.7 ly
(83.8 ± 0.2 pc)
Absolute magnitude (MV)2.10[3]
Details
Rotational velocity (v sin i)
21.3±1.0[11] km/s
PPM 195288, WDS J12143-0543A[12]
Database references
SIMBADdata

FG Virginis is a well-studied

lunar occultations.[13]

The variability of this star was first reported by

pulsating stars in the instability strip.[14] It was subsequently grouped in the class of Delta Scuti variables, which show a pulsation period of less than a day.[15] Observations in 1984 by P. Lopez de Coca showed at least one pulsation period with a cycle of 1.9 hours.[16] L. Mantegazza and associates in 1994 were able to detect seven or more pulsation modes, with the previously detected dominant mode being a radial pulsation with a frequency of 12.72 cycles per day.[17]

The star became of interest to

astroseismology study because of its relatively slow rotation rate and the numerous modes of pulsation. A multi-site campaign involving the Whole Earth Telescope network was conducted in 1993 to observe this star, which detected ten modes.[1] This was increased to 24 frequencies in 1998,[18] then 67 independent frequencies with 79 total by 2005. Evidence suggests there are many more such modes.[19]

This is an

projected rotational velocity of 21 km/s, but the actual rotational velocity is likely much higher at around 80 km/s.[11]

References

Further reading