AC Andromedae

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AC Andromedae
ACAndLightCurve.png
A visual band light curve of AC Andromedae, from data presented by Peña et al. [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Andromeda
Right ascension 23h 18m 02.34605s [2]
Declination +48° 46 58.3403 [2]
Apparent magnitude  (V)10.7 11.9 variable [3]
Characteristics
Spectral type F5 [4]
Apparent magnitude  (B)11.48 [5]
Apparent magnitude  (V)10.90 [5]
Apparent magnitude  (G)10.9002 [2]
Apparent magnitude  (J)9.646 [6]
Apparent magnitude  (H)9.483 [6]
Apparent magnitude  (K)9.345 [6]
B−V color index 0.5389 [5]
Variable type Peculiar [3]
Astrometry
Radial velocity (Rv)−50.0±2.8 [7]  km/s
Proper motion (μ)RA: −2.160±0.012 [2]   mas/yr
Dec.: −2.345±0.013 [2]   mas/yr
Parallax (π)0.4948 ± 0.0138  mas [2]
Distance 6,600 ± 200  ly
(2,020 ± 60  pc)
Absolute magnitude  (MV)−0.82 [4]
Details
Mass 3.4 [2]   M
Radius 11 [2]   R
Luminosity 170 [2]   L
Surface gravity (log g)2.76 [8]   cgs
Temperature 6,315 [9]   K
Metallicity [Fe/H]−1.46 [8]   dex
Age 271 [2]   Myr
Other designations
2MASS J23180234+4846582, BD+47 4104, HIP  115046, TYC 3644-2114-1
Database references
SIMBAD data

AC Andromedae (AC And) is a variable star in the constellation Andromeda. Its maximum apparent visual magnitude is 10.77, but can be seen fainter down to a magnitude of 11.9.

AC Andromedae was first reported to be a variable star by Paul Guthnick and Richard Prager in 1927. They noted that it varied in brightness rapidly, with no discernible period. [10] [11]

The nature of AC Andromedae is still not determined. Its light curve shows clearly three radial pulsation modes, the fundamental one with a period of 0.71 days, and the first two overtones of 0.525 and 0.421 days, respectively. It is then unclear if it belongs to the class of RR Lyrae variables or to the one of Delta Scuti variables. [12] [13] Another study points at AC And as an intermediate object between classical Cepheids and Delta Scuti variables. [4] The physical parameters of the star itself would be different depending on which class it belongs to.

By late 2018, the AC Andromedae was classified as rare "triple-mode" subtype of the dwarf cepheid (high-amplitude Delta Scuti variable). [14] [15]

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References

  1. Peña, J. H.; Peniche, R.; Hobart, M. A.; de la Cruz, C.; Gallegos, A. A. (2005). "Uvby-β Photometry of the RR Lyrae Star AC and". Revista Mexicana de Astronomía y Astrofísica. 41: 461. Bibcode:2005RMxAA..41..461P.
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  3. 1 2 AC And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2018-10-17.
  4. 1 2 3 Fernie, J. D. (November 1994). "AC Andromedae: the missing link between δ Scuti stars and classical Cepheids?". Monthly Notices of the Royal Astronomical Society. 271: L19–L20. Bibcode:1994MNRAS.271L..19F. doi: 10.1093/mnras/271.1.L19 .
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  11. Münch, Guido (1951). "On the Spectrum of AC Andromedae". The Astrophysical Journal. 114: 546. Bibcode:1951ApJ...114..546M. doi: 10.1086/145499 .
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