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Delta3 Tauri

From Wikipedia, the free encyclopedia
Star in the constellation Taurus
For other stars with thisBayer designation, seeδ Tauri.
δ3 Tauri

Location of δ3 Tauri in theHyades, indicated by itsFlamsteed designation 68
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationTaurus
Right ascension04h 25m 29.38340s[1]
Declination+17° 55′ 40.4579″[1]
Apparent magnitude (V)+4.32 (4.35 + 8.37)[2]
Characteristics
Spectral typeA2IV-Vs[3]
Astrometry
Proper motion (μ)RA: +41.91[1]mas/yr
Dec.: −34.54[1]mas/yr
Parallax (π)21.96±0.51 mas[1]
Distance149 ± 3 ly
(46 ± 1 pc)
Absolute magnitude (MV)+1.14[4]
Details
Mass2.27±0.23[5] M
Radius2.4[6] R
Luminosity29.5[5] L
Surface gravity (log g)3.95[5] cgs
Temperature9,025[5] K
Metallicity [Fe/H]+0.32[7] dex
Rotation2.13[8] days
Rotational velocity (v sin i)11.3[5] km/s
Age630[9] Myr
Other designations
Cleeia,δ3 Tau,68 Tauri,BD+17°719,HD 27962,HIP 20648,HR 1389,SAO 93923,ADS 3206[10]
Database references
SIMBADdata

Delta3 Tauri (δ3 Tauri) is abinary star[2] system in thezodiacconstellation ofTaurus. Based upon an annualparallax shift of 21.96 mas as seen from Earth,[1] it is located roughly 149 light years distant from theSun. It is visible to the naked eye with a combinedapparent visual magnitude of +4.32.[2] δ3 Tauri is separated from δ1 Tauri by 0.72° on the sky.[10] This star also has the traditional Latin nameCleeia,[11][12] from theGreekKleeia (transliteration of Κλεεια),[13] who was one of theHyades sisters. It is considered a member of theHyades cluster.[5]

InChinese,畢宿 (Bì Xiù), meaningNet, refers to an asterism consisting δ3 Tauri,ε Tauri,δ1 Tauri,γ Tauri,Aldebaran,71 Tauri andλ Tauri.[14] Consequently, theChinese name for δ3 Tauri itself is畢宿二 (Bì Xiù èr), "the Second Star of Net".[15]

The magnitude 4.35[2] primary, component A, appears to be anA-type star intermediate betweenmain sequence andsubgiant, with astellar classification of A2 IV-Vs. The "s" indicates sharp (unusually narrow)absorption lines, a sign of slow rotation. It is a candidateblue straggler and shows characteristics of anAm star. Abt (1985) gave it a classification of A2kA3hA5m, indicating that thespectrum displays thecalcium K-line of an A2 star, thehydrogen lines of an A3 star and themetal lines of an A5 star. It is deficient in scandium but has enhancediron peak and heavy elements.[5] Although suspected ofvariability in the past,[16] Delta3 Tauri A was subsequently determined to bephotometrically constant.[17]

The companion, component B, is a magnitude 8.37[2] star at anangular separation of 1.80 arc seconds along aposition angle of 341°, as of 2010. At 77arcseconds away (as of 2006) is a magnitude 11.12visual companion, designated component C.[18]

References

[edit]
  1. ^abcdefvan 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. ^abcdeEggleton, 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.
  3. ^Gray, R. O.; Garrison, R. F. (1987), "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation",The Astrophysical Journal Supplement Series,65: 581,Bibcode:1987ApJS...65..581G,doi:10.1086/191237.
  4. ^Eggen, Olin J. (July 1998), "The Age Range of Hyades Stars",The Astronomical Journal,116 (1):284–292,Bibcode:1998AJ....116..284E,doi:10.1086/300413.
  5. ^abcdefgGebran, M.; Vick, M.; Monier, R.; Fossati, L. (November 2010), "Chemical composition of A and F dwarfs members of the Hyades open cluster",Astronomy and Astrophysics,523: 13,arXiv:1006.5284,Bibcode:2010A&A...523A..71G,doi:10.1051/0004-6361/200913273,S2CID 7164596, A71.
  6. ^Stassun, Keivan G.; et al. (2019), "The Revised TESS Input Catalog and Candidate Target List",The Astronomical Journal,158 (4): 138,arXiv:1905.10694,Bibcode:2019AJ....158..138S,doi:10.3847/1538-3881/ab3467.
  7. ^Gáspár, András; Rieke, George H.; Ballering, Nicholas (2016), "The Correlation between Metallicity and Debris Disk Mass",The Astrophysical Journal,826 (2): 171,arXiv:1604.07403,Bibcode:2016ApJ...826..171G,doi:10.3847/0004-637X/826/2/171.
  8. ^Bychkov, V. D.; Bychkova, L. V.; Madej, J. (2005), "A catalog of stellar magnetic rotational phase curves",Astronomy and Astrophysics,430 (3): 1143,Bibcode:2005A&A...430.1143B,doi:10.1051/0004-6361:20034563.
  9. ^De Rosa, R. J.; Patience, J.; Wilson, P. A.; Schneider, A.; Wiktorowicz, S. J.; Vigan, A.; Marois, C.; Song, I.; MacIntosh, B.; Graham, J. R.; Doyon, R.; Bessell, M. S.; Thomas, S.; Lai, O. (2014), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc",Monthly Notices of the Royal Astronomical Society,437 (2): 1216,arXiv:1311.7141,Bibcode:2014MNRAS.437.1216D,doi:10.1093/mnras/stt1932.
  10. ^ab"del03 Tau",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-08-07.
  11. ^Falkner, David E. (2011),The Mythology of the Night Sky: An Amateur Astronomer's Guide to the Ancient Greek and Roman Legends, The Patrick Moore Practical Astronomy Series,Springer Science & Business Media, p. 36,ISBN 978-1461401377.
  12. ^Bagnall, Philip M. (2012),The Star Atlas Companion: What you need to know about the Constellations, Springer Praxis Books, Springer Science & Business Media, p. 422,Bibcode:2012sacw.book.....B,ISBN 978-1461408307.
  13. ^"Family of the Hyades",Theoi Greek Mythology, retrieved2017-08-08.
  14. ^(in Chinese)中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005,ISBN 978-986-7332-25-7.
  15. ^(in Chinese)香港太空館 - 研究資源 - 亮星中英對照表Archived 2008-10-25 at theWayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
  16. ^Kholopov, P. N.; et al. (February 1981), "65th Name-List of Variable Stars",Information Bulletin on Variable Stars,1921: 1,Bibcode:1981IBVS.1921....1K.
  17. ^Adelman, S. J. (June 1997), "On the possible variability of metallic-line and Mercury-Manganese stars",Astronomy & Astrophysics Supplement Series,123 (3):445–447,Bibcode:1997A&AS..123..445A,doi:10.1051/aas:1997167.
  18. ^Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6):3466–3471,Bibcode:2001AJ....122.3466M,doi:10.1086/323920.
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