V529 Andromedae

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V529 Andromedae
V529AndLightCurve.png
Blue band light curves for V529 Andromedae, adapted from Henry and Fekel (2005) [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Andromeda
Right ascension 01h 27m 26.6729s [2]
Declination +41° 06 04.178 [2]
Apparent magnitude  (V)6.46 [3]
Characteristics
Spectral type Am(kA5/hF1/mF2) [4]
U−B color index 0.03 [3]
B−V color index 0.27 [3]
V−R color index 0.26 [3]
R−I color index 0.16 [3]
Variable type γ Doradus and δ Scuti [5]
Astrometry
Radial velocity (Rv)0.8±0.3 [1]  km/s
Proper motion (μ)RA: 9.611±0.030 [2]   mas/yr
Dec.: 25.910±0.024 [2]   mas/yr
Parallax (π)18.7624 ± 0.0298  mas [2]
Distance 173.8 ± 0.3  ly
(53.30 ± 0.08  pc)
Absolute magnitude  (MV)+2.68 [1]
Details
Mass 1.55±0.1 [1]   M
Radius 1.7±0.1 [1]   R
Luminosity 6.5±0.6 [1]   L
Surface gravity (log g)4.1±0.2 [5]   cgs
Temperature 7560±180 [5]   K
Metallicity +0.11 [6]
Rotational velocity (v sin i)53.1±0.5 [5]  km/s
Age 727 [2]   Myr
Other designations
SAO 37227, HIP 6794, HR 418, HD 8801, BD+40°289
Database references
SIMBAD data

V529 Andromedae, also known as HD 8801, is a variable star in the constellation of Andromeda. It has a 13th magnitude visual companion star 15" away, which is just a distant star on the same line of sight.

Contents

It is also an Am star with a spectral classification Am(kA5/hF1/mF2), meaning that it has the calcium K line of a star with spectral type A5, the Balmer series of a F1 star, and metallic lines of an F2 star. [4]

Variability

V529 Andromedae was the first star known to combine Gamma Doradus and Delta Scuti type pulsations. [1] Nine different pulsation frequencies have been observed, and three of them could arise from a previously unknown stellar pulsation mode. [7]

Companion

V529 Andromedae has a 13th magnitude companion about 15 away. [8] It is a far more distant star than V529 Andromedae, only coincidentally aligned in the sky. [9]

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<span class="mw-page-title-main">Gamma Doradus variable</span> Type of variable star

Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically young, early F or late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day. This class of variable stars is relatively new, having been first characterized in the second half of the 1990s, and details on the underlying physical cause of the variations remains under investigation.

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References

  1. 1 2 3 4 5 6 7 Henry, Gregory W.; Fekel, Francis C. (2005). "HD 8801: A Unique Single Am Star with γ Doradus and δ Scuti Pulsations". The Astronomical Journal. 129 (4): 2026–2033. Bibcode:2005AJ....129.2026H. CiteSeerX   10.1.1.145.5743 . doi:10.1086/428373. S2CID   16975954.
  2. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics . arXiv: 2208.00211 . doi: 10.1051/0004-6361/202243940 . Gaia DR3 record for this source at VizieR.
  3. 1 2 3 4 5 Mendoza, E. E.; et al. (1978). "UBVRI photometry of 225 AM stars". The Astronomical Journal. 83: 606–614. Bibcode:1978AJ.....83..606M. doi:10.1086/112242.
  4. 1 2 Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135–172. Bibcode:1995ApJS...99..135A. doi:10.1086/192182.
  5. 1 2 3 4 Neuteufel, R.; et al. (2013). "Abundance analysis of the γ Doradus-δ Scuti hybrid metallic line (Am) star HD 8801". Astronomische Nachrichten. 334 (7): 638–647. arXiv: 1307.3497 . Bibcode:2013AN....334..638N. doi:10.1002/asna.201311909. S2CID   117570505.
  6. Ghazaryan, S.; Alecian, G.; Hakobyan, A. A. (2018). "New catalogue of chemically peculiar stars, and statistical analysis". Monthly Notices of the Royal Astronomical Society. 480 (3): 2953–2962. arXiv: 1807.06902 . Bibcode:2018MNRAS.480.2953G. doi:10.1093/mnras/sty1912. S2CID   119062018.
  7. Handler, G. (2009). "Confirmation of simultaneous p and g mode excitation in HD 8801 and γ Peg from time-resolved multicolour photometry of six candidate 'hybrid' pulsators". Monthly Notices of the Royal Astronomical Society. 398 (3): 1339–1351. arXiv: 0904.4859 . Bibcode:2009MNRAS.398.1339H. doi:10.1111/j.1365-2966.2009.15005.x. S2CID   18019973.
  8. Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi: 10.1086/323920 .
  9. Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics . arXiv: 2208.00211 . doi: 10.1051/0004-6361/202243940 . Gaia DR3 record for this source at VizieR.