Lambda Boötis

Lambda Boötis (λ Boötis, abbreviated Lam Boo, λ Boo), also named Xuange[10] (/ˈʃwɛnɡə/), is a star in the northern constellation of Boötes. Based on parallax measurements, it is approximately 99 light-years from the Sun.[1]

λ Boötis
Location of λ Boötis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Boötes
Right ascension 14h 16m 23.01880s[1]
Declination +46° 05′ 17.9005″[1]
Apparent magnitude (V) +4.18[2]
Characteristics
Spectral type A0p λB[3]
U−B color index +0.05[2]
B−V color index +0.08[2]
Astrometry
Radial velocity (Rv)−7.9±1.6[4] km/s
Proper motion (μ) RA: −187.33±0.14[1] mas/yr
Dec.: 159.05±0.11[1] mas/yr
Parallax (π)32.94 ± 0.16[1] mas
Distance99.0 ± 0.5 ly
(30.4 ± 0.1 pc)
Absolute magnitude (MV)+1.71±0.23[5]
Details
Mass1.66+0.19
−0.16[6] M☉
Radius1.7[7] R☉
Luminosity19.1+9.0
−6.1[6] L☉
Surface gravity (log g)4.188[8] cgs
Temperature8720[9] K
Rotational velocity (v sin i)100[8] km/s
Age2.8+1.1
−0.8[6] Gyr
Other designations
Xuange, λ Boo, 19 Boötis, BD+46° 1949, FK5 527, GC 19273, GJ 3837, HD 125162, HIP 69732, HR 5351, SAO 44965
Database references
SIMBADdata

Lambda Boötis is a white A-type main sequence dwarf with an apparent magnitude of +4.18. It is the prototype of a group of rare stars known as Lambda Boötis stars, all of which are dwarf stars with unusually low abundances of metals in their spectra. Its diameter has been directly measured to be 1.7 times that of the Sun.[7]

Nomenclature

λ Boötis (Latinised to Lambda Boötis) is the star's Bayer designation.

In Chinese astronomy, Lambda Boötis is called 玄戈, Pinyin: Xuángē, meaning 'sombre lance', because this star is marking itself and standing alone in the Sombre Lance asterism, Purple Forbidden enclosure (see : Chinese constellations).[11] 玄戈 (Xuángē) westernized into Heuen Ko, but that name was assigned to Gamma Boötis by R.H. Allen, with the meaning of 'the heavenly spear'.[12] In 2016, the IAU organized a Working Group on Star Names (WGSN)[13] to catalog and standardize proper names for stars. The WGSN approved the name Xuange for Lambda Boötis on 30 June 2017 and it is now so included in the List of IAU-approved Star Names.[10]

This star, along with the Aselli (Theta Boötis, Iota Boötis and Kappa Boötis), were Al Aulād al Dhiʼbah (ألعولد ألذعب - al aulād al dhiʼb), "the Whelps of the Hyenas".[14] Al Aulād al Dhiʼbah or Aulad al Thiba was the title of this star in a 1971 NASA memorandum.[15]

References
  1. van 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. Vizier catalog entry
  2. Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99): 99. Bibcode:1966CoLPL...4...99J.
  3. Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". Astrophysical Journal Supplement. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182.
  4. Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  5. Paunzen, E.; et al. (November 2002). "The status of Galactic field λ Bootis stars in the post-Hipparcos era". Monthly Notices of the Royal Astronomical Society. 336 (3): 1030–1042. arXiv:astro-ph/0207488. Bibcode:2002MNRAS.336.1030P. doi:10.1046/j.1365-8711.2002.05865.x. S2CID 2389489.
  6. Montesinos, B.; et al. (March 2009), "Parameters of Herbig Ae/Be and Vega-type stars", Astronomy and Astrophysics, 495 (3): 901–917, arXiv:0811.3557, Bibcode:2009A&A...495..901M, doi:10.1051/0004-6361:200810623, S2CID 14972955
  7. Ciardi; et al. (2007), "The Angular Diameter of λ Boötis", The Astrophysical Journal, 659 (2): 1623–1628, arXiv:astro-ph/0612723, Bibcode:2007ApJ...659.1623C, doi:10.1086/512077, S2CID 17861605
  8. Song, Inseok; Caillault, J.-P.; Barrado y Navascués, David; Stauffer, John R. (February 2001), "Ages of A-Type Vega-like Stars from uvbyβ Photometry", The Astrophysical Journal, 546 (1): 352–357, arXiv:astro-ph/0010102, Bibcode:2001ApJ...546..352S, doi:10.1086/318269, S2CID 18154947
  9. Martínez-Galarza, J. R.; et al. (March 2009), "Infrared Emission by Dust Around λ Bootis Stars: Debris Disks or Thermally Emitting Nebulae?", The Astrophysical Journal, 694 (1): 165–173, arXiv:0812.2198, Bibcode:2009ApJ...694..165M, doi:10.1088/0004-637X/694/1/165, S2CID 14298654
  10. "Naming Stars". IAU.org. Retrieved 16 December 2017.
  11. (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 14 日
  12. Richard Hinckley Allen: Star Names — Their Lore and Meaning: Boötes
  13. "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
  14. Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York, NY: Dover Publications Inc, p. 105, ISBN 978-0-486-21079-7, retrieved 2010-12-12
  15. Jack W. Rhoads - Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propulsion Laboratory, California Institute of Technology; November 15, 1971
  • Hoffleit; et al. (1991), "HR 5351", Bright Star Catalogue (5th Revised ed.), retrieved 2017-09-13.
  • "lam Bo0", Aladin previewer, Centre de Données astronomiques de Strasbourg, retrieved 2017-09-12.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.