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Tau2 Hydrae

From Wikipedia, the free encyclopedia
Binary star system in the constellation Hydra
For other stars with this Bayer designation, seeτ Hydrae.
Tau2 Hydrae
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationHydra
Right ascension09h 31m 58.92729s[1]
Declination−01° 11′ 04.7899″[1]
Apparent magnitude (V)+4.56[2]
Characteristics
Spectral typeA3 V[3]
U−Bcolor index+0.06[2]
B−Vcolor index+0.11[2]
Variable typeSuspected[4]
Astrometry
Radial velocity (Rv)+3.9±0.4[5] km/s
Proper motion (μ)RA: −12.60[1]mas/yr
Dec.: −3.99[1]mas/yr
Parallax (π)6.30±0.72 mas[1]
Distanceapprox. 520 ly
(approx. 160 pc)
Absolute magnitude (MV)−1.43[6]
Details
Radius4.5[7] R
Luminosity285[8] L
Temperature7,918[8] K
Rotational velocity (v sin i)54.0±0.6[3] km/s
Other designations
Ukdah,τ2 Hya,32 Hydrae,BD−00°2211,HD 82446,HIP 46776,HR 3787,SAO 136932.[9]
Database references
SIMBADdata

Tau2 Hydrae is a probableastrometric binary[10] star system in the equatorialconstellation ofHydra. Based upon an annualparallax shift of 6.30 mas as seen from Earth, it is located around 520 light years from theSun. The brighter component is visible to the naked eye with anapparent visual magnitude of +4.56.[2]

The primary member, component A, is anA-type main sequence star with astellar classification of A3 V.[3] It is asuspected variable of unknown type, with anamplitude of 0.06 in visual magnitude.[4] The star has around 4.5[7] times theradius of the Sun and is radiating about 285 times thesolar luminosity from itsphotosphere at aneffective temperature of 7,918 K.[8]

References

[edit]
  1. ^abcdevan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abcDíaz, C. G.; et al. (July 2011), "Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum",Astronomy & Astrophysics,531: A143,arXiv:1012.4858,Bibcode:2011A&A...531A.143D,doi:10.1051/0004-6361/201016386,S2CID 119286673.
  4. ^abAdelman, S. J. (October 2000), "On the Variability of A3-F0 Luminosity Class III-V Stars",Information Bulletin on Variable Stars,4969 (4969): 1,Bibcode:2000IBVS.4969....1A.
  5. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  7. ^abPasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (3rd ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^abcMcDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–57,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  9. ^"* tau02 Hya".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-03-22.{{cite web}}: CS1 maint: postscript (link)
  10. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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