Astronomy:V471 Tauri

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Short description: Variable star in the constellation Taurus
V471 Tauri
V471TauLightCurve.png
A light curve for V471 Tauri, plotted from TESS data[1]
Observation data
Equinox J2000.0]] (ICRS)
Constellation Taurus
Right ascension  03h 50m 24.9667s[2]
Declination 17° 14′ 47.431″[2]
Apparent magnitude (V) 9.40 - 9.71[3]
Characteristics
Evolutionary stage K2V + D2[4]
Variable type Algol + RS CVn[3]
Astrometry
Radial velocity (Rv)37.4±0.5[5] km/s
Proper motion (μ) RA: 127.278[2] mas/yr
Dec.: −22.321[2] mas/yr
Parallax (π)21.0129 ± 0.0158[2] mas
Distance155.2 ± 0.1 ly
(47.59 ± 0.04 pc)
Orbit[6]
Period (P)0.52118 days
Semi-major axis (a)0.01496 AU
Eccentricity (e)0 (assumed)
Inclination (i)80.8°
Details
White dwarf
Mass0.792[6] M
Radius0.01134[6] R
Luminosity0.145[7] L
Surface gravity (log g)8.227[6] cgs
Temperature34,500[7] K
K star
Mass0.852[6] M
Radius0.816[6] R
Luminosity0.41[8] L
Surface gravity (log g)4.49[9] cgs
Temperature5,066[9] K
Rotation0.5211 days[8]
Rotational velocity (v sin i)89.30[9] km/s
Age625[9] Myr
Other designations
Database references
SIMBADdata

V471 Tauri (short V471 Tau) is a eclipsing variable star in the constellation of Taurus. The star has a visual magnitude of 9 which makes it impossible to see with the naked eye. It is around 155 light-years away from the Solar System.

Physical properties

The V471 Tauri system has at least two members: a white dwarf star of spectral type D2; and a K-type main sequence star (K2 V). There are variations in the timing of the eclipses that were once thought to be due to a third member of the system, proposed to be a brown dwarf, but this has been ruled out and the eclipse variations may be caused by the Applegate mechanism. The system is located in the Hyades star cluster.[6]

References

  1. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html. 
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 Samus, N. N. et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1 61 (1): 80–88. doi:10.1134/S1063772917010085. Bibcode2017ARep...61...80S. 
  4. Hussain, G. A. J.; Allende Prieto, C.; Saar, S. H.; Still, M. (2006). "Spot patterns and differential rotation in the eclipsing pre-cataclysmic variable binary, V471 Tau". Monthly Notices of the Royal Astronomical Society 367 (4): 1699–1708. doi:10.1111/j.1365-2966.2006.10073.x. Bibcode2006MNRAS.367.1699H. 
  5. Karataș, Yüksel; Bilir, Selçuk; Eker, Zeki; Demircan, Osman; Liebert, James; Hawley, Suzanne L.; Fraser, Oliver J.; Covey, Kevin R. et al. (2004). "Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution". Monthly Notices of the Royal Astronomical Society 349 (3): 1069–1092. doi:10.1111/j.1365-2966.2004.07588.x. Bibcode2004MNRAS.349.1069K. 
  6. 6.0 6.1 6.2 6.3 6.4 6.5 6.6 Muirhead, Philip S.; Nordhaus, Jason; Drout, Maria R. (2022). "Revised Stellar Parameters for V471 Tau, A Post-common Envelope Binary in the Hyades". The Astronomical Journal 163 (1): 34. doi:10.3847/1538-3881/ac390f. Bibcode2022AJ....163...34M. 
  7. 7.0 7.1 Vaccaro, T. R.; Wilson, R. E.; Van Hamme, W.; Terrell, Dirk (2015). "The V471 Tauri System: A Multi-data-type Probe". The Astrophysical Journal 810 (2): 157. doi:10.1088/0004-637X/810/2/157. Bibcode2015ApJ...810..157V. 
  8. 8.0 8.1 Kővári, Zs; Kriskovics, L.; Oláh, K.; Odert, P.; Leitzinger, M.; Seli, B.; Vida, K.; Borkovits, T. et al. (2021). "A confined dynamo: Magnetic activity of the K-dwarf component in the pre-cataclysmic binary system V471 Tauri". Astronomy and Astrophysics 650: A158. doi:10.1051/0004-6361/202140707. Bibcode2021A&A...650A.158K. 
  9. 9.0 9.1 9.2 9.3 Zaire, B.; Donati, J. -F.; Klein, B. (2021). "Magnetic field and activity phenomena of the K2 dwarf V471 Tau". Monthly Notices of the Royal Astronomical Society 504 (2): 1969. doi:10.1093/mnras/stab1019. Bibcode2021MNRAS.504.1969Z.