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Xi Cephei

Xi Cephei (ξ Cephei, abbreviated Xi Cep, ξ Cep) is a multiple star system in the constellation of Cepheus. It is approximately 86 light-years from Earth.[6]

ξ Cephei
Location of ξ Cephei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 22h 03m 47.455s[1]
Declination +64° 37′ 40.71″[1]
Apparent magnitude (V) 4.2[2] (4.45 + 4.60[3])
Characteristics
ξ Cephei A
Spectral type kA2.5hF2mF2(IV)[4]
ξ Cephei B
Spectral type F8V[5]
Astrometry
Proper motion (μ) RA: 215.46±1.14[1] mas/yr
Dec.: 91.06±0.97[1] mas/yr
Parallax (π)38.10 ± 2.81 mas[6]
Distance86 ± 6 ly
(26 ± 2 pc)
Absolute magnitude (MV)+1.79[7]
Orbit[8]
Period (P)810.9 d
Eccentricity (e)0.46
Periastron epoch (T)2438529.8 JD
Argument of periastron (ω)
(secondary)
106°
Semi-amplitude (K1)
(primary)
7.1 km/s
Semi-amplitude (K2)
(secondary)
19.9 km/s
Details
ξ Cephei Aa
Mass1.045±0.031[6] M
ξ Cephei Ab
Mass0.408±0.066[6] M
Other designations
Kurhah, 17 Cephei, BD+63°1802, CCDM J22038+2407, HIP 108917, HR 8417, SAO 19827, WDS J22038+6438
A: HD 209790
B: HD 209791
Database references
SIMBADξ
A
B

It consists of two binary stars, designated Xi Cephei A and B, together with a more distant companion, Xi Cephei C. A's two components are themselves designated Xi Cephei Aa (officially named Kurhah /ˈkɜːrhə/, the traditional name of the system)[9] and Ab.

Nomenclature edit

ξ Cephei (Latinised to Xi Cephei) is the system's Bayer designation. The designations of the three constituents as ξ Cephei A, B and C, and those of A's components - ξ Cephei Aa and Ab - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[10]

Xi Cephei bore the traditional names Kurhah, Alkirdah or Al Kirduh,[11] the name coming from Qazvini who gave Al Ḳurḥaḥ (القرحة al-qurhah), an Arabic word Ideler translated as a white spot, or blaze, in the face of a horse. Allen indicates that Ideler felt this was not a proper name for a star, and suggested the name Al Ḳirdah (ألقردة al qírada "the Ape").[12] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[13] to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[14] It approved the name Kurhah for the component Xi Cephei Aa on 12 September 2016 and it is now so included in the List of IAU-approved Star Names.[9]

In Chinese, 天鈎 (Tiān Gōu), meaning Celestial Hook, refers to an asterism consisting of Xi Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Alpha Cephei, 26 Cephei, Iota Cephei and Omicron Cephei.[15] Consequently, the Chinese name for Xi Cephei itself is 天鈎六 (Tiān Gōu liù, English: the Sixth Star of Celestial Hook).[16]

Properties edit

Xi Cephei A is a double-lined spectroscopic binary system with an orbital period of 810.9 days and an eccentricity of 0.46.[8] The primary, component Aa, is a chemically peculiar Am star, a probable subgiant with an apparent magnitude of +4.29. Eight arcseconds away, Xi Cephei B is another spectroscopic binary. Xi Cephei C is a 13th magnitude star nearly two arcminutes away.[3]

References edit

  1. ^ a b c d 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. ^ Monet, David G.; Levine, Stephen E.; Canzian, Blaise; Ables, Harold D.; Bird, Alan R.; Dahn, Conard C.; Guetter, Harry H.; Harris, Hugh C.; Henden, Arne A.; Leggett, Sandy K.; Levison, Harold F.; Luginbuhl, Christian B.; Martini, Joan; Monet, Alice K. B.; Munn, Jeffrey A.; Pier, Jeffrey R.; Rhodes, Albert R.; Riepe, Betty; Sell, Stephen; Stone, Ronald C.; Vrba, Frederick J.; Walker, Richard L.; Westerhout, Gart; Brucato, Robert J.; Reid, I. Neill; Schoening, William; Hartley, M.; Read, M. A.; Tritton, S. B. (2003). "The USNO-B Catalog". The Astronomical Journal. 125 (2): 984–993. arXiv:astro-ph/0210694. Bibcode:2003AJ....125..984M. doi:10.1086/345888. S2CID 55896673.
  3. ^ a b 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.
  4. ^ Gray, R. O; Garrison, R. F (1989). "The early F-type stars - Refined classification, confrontation with Stromgren photometry, and the effects of rotation". The Astrophysical Journal Supplement Series. 69: 301. Bibcode:1989ApJS...69..301G. doi:10.1086/191315.
  5. ^ Gray, R. O; Napier, M. G; Winkler, L. I (2001). "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars". The Astronomical Journal. 121 (4): 2148. Bibcode:2001AJ....121.2148G. doi:10.1086/319956.
  6. ^ a b c d Farrington, C. D.; et al. (2014). "Separated Fringe Packet Observations with the CHARA Array. II. omega Andromeda, HD 178911, and xi Cephei". The Astronomical Journal. 148 (3): 48. arXiv:1407.0639. Bibcode:2014AJ....148...48F. doi:10.1088/0004-6256/148/3/48. S2CID 12909818.
  7. ^ 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.
  8. ^ a b Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; et al. (2004), "SB9: The ninth catalogue of spectroscopic binary orbits", Astronomy & Astrophysics, 424 (2): 727–732, arXiv:astro-ph/0406573, Bibcode:2004A&A...424..727P, doi:10.1051/0004-6361:20041213, S2CID 119387088.
  9. ^ a b "Naming Stars". IAU.org. Retrieved 16 December 2017.
  10. ^ Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR].
  11. ^ . Archived from the original on 2008-02-02. Retrieved 2010-12-08.
  12. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 159. ISBN 0-486-21079-0. Retrieved 2010-12-12.
  13. ^ IAU Working Group on Star Names (WGSN), International Astronomical Union, retrieved 22 May 2016.
  14. ^ "WG Triennial Report (2015-2018) - Star Names" (PDF). p. 5. Retrieved 2018-07-14.
  15. ^ (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.
  16. ^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 January 29, 2011, at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.

cephei, cephei, abbreviated, multiple, star, system, constellation, cepheus, approximately, light, years, from, earth, cepheilocation, cephei, circled, observation, dataepoch, j2000, equinox, j2000, constellation, cepheus, right, ascension, 455s, declination, . Xi Cephei 3 Cephei abbreviated Xi Cep 3 Cep is a multiple star system in the constellation of Cepheus It is approximately 86 light years from Earth 6 3 CepheiLocation of 3 Cephei circled Observation dataEpoch J2000 Equinox J2000 Constellation Cepheus Right ascension 22h 03m 47 455s 1 Declination 64 37 40 71 1 Apparent magnitude V 4 2 2 4 45 4 60 3 Characteristics 3 Cephei A Spectral type kA2 5hF2mF2 IV 4 3 Cephei B Spectral type F8V 5 AstrometryProper motion m RA 215 46 1 14 1 mas yr Dec 91 06 0 97 1 mas yrParallax p 38 10 2 81 mas 6 Distance86 6 ly 26 2 pc Absolute magnitude MV 1 79 7 Orbit 8 Period P 810 9 dEccentricity e 0 46Periastron epoch T 2438529 8 JDArgument of periastron w secondary 106 Semi amplitude K1 primary 7 1 km sSemi amplitude K2 secondary 19 9 km s Details3 Cephei AaMass1 045 0 031 6 M 3 Cephei AbMass0 408 0 066 6 M Other designationsKurhah 17 Cephei BD 63 1802 CCDM J22038 2407 HIP 108917 HR 8417 SAO 19827 WDS J22038 6438A HD 209790B HD 209791 Database referencesSIMBAD3AB It consists of two binary stars designated Xi Cephei A and B together with a more distant companion Xi Cephei C A s two components are themselves designated Xi Cephei Aa officially named Kurhah ˈ k ɜːr h e the traditional name of the system 9 and Ab Nomenclature edit3 Cephei Latinised to Xi Cephei is the system s Bayer designation The designations of the three constituents as 3 Cephei A B and C and those of A s components 3 Cephei Aa and Ab derive from the convention used by the Washington Multiplicity Catalog WMC for multiple star systems and adopted by the International Astronomical Union IAU 10 Xi Cephei bore the traditional names Kurhah Alkirdah or Al Kirduh 11 the name coming from Qazvini who gave Al Ḳurḥaḥ القرحة al qurhah an Arabic word Ideler translated as a white spot or blaze in the face of a horse Allen indicates that Ideler felt this was not a proper name for a star and suggested the name Al Ḳirdah ألقردة al qirada the Ape 12 In 2016 the International Astronomical Union organized a Working Group on Star Names WGSN 13 to catalogue and standardize proper names for stars The WGSN decided to attribute proper names to individual stars rather than entire multiple systems 14 It approved the name Kurhah for the component Xi Cephei Aa on 12 September 2016 and it is now so included in the List of IAU approved Star Names 9 In Chinese 天鈎 Tian Gōu meaning Celestial Hook refers to an asterism consisting of Xi Cephei 4 Cephei HD 194298 Eta Cephei Theta Cephei Alpha Cephei 26 Cephei Iota Cephei and Omicron Cephei 15 Consequently the Chinese name for Xi Cephei itself is 天鈎六 Tian Gōu liu English the Sixth Star of Celestial Hook 16 Properties editXi Cephei A is a double lined spectroscopic binary system with an orbital period of 810 9 days and an eccentricity of 0 46 8 The primary component Aa is a chemically peculiar Am star a probable subgiant with an apparent magnitude of 4 29 Eight arcseconds away Xi Cephei B is another spectroscopic binary Xi Cephei C is a 13th magnitude star nearly two arcminutes away 3 References edit a b c d van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 Vizier catalog entry Monet David G Levine Stephen E Canzian Blaise Ables Harold D Bird Alan R Dahn Conard C Guetter Harry H Harris Hugh C Henden Arne A Leggett Sandy K Levison Harold F Luginbuhl Christian B Martini Joan Monet Alice K B Munn Jeffrey A Pier Jeffrey R Rhodes Albert R Riepe Betty Sell Stephen Stone Ronald C Vrba Frederick J Walker Richard L Westerhout Gart Brucato Robert J Reid I Neill Schoening William Hartley M Read M A Tritton S B 2003 The USNO B Catalog The Astronomical Journal 125 2 984 993 arXiv astro ph 0210694 Bibcode 2003AJ 125 984M doi 10 1086 345888 S2CID 55896673 a b 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 Gray R O Garrison R F 1989 The early F type stars Refined classification confrontation with Stromgren photometry and the effects of rotation The Astrophysical Journal Supplement Series 69 301 Bibcode 1989ApJS 69 301G doi 10 1086 191315 Gray R O Napier M G Winkler L I 2001 The Physical Basis of Luminosity Classification in the Late A F and Early G Type Stars I Precise Spectral Types for 372 Stars The Astronomical Journal 121 4 2148 Bibcode 2001AJ 121 2148G doi 10 1086 319956 a b c d Farrington C D et al 2014 Separated Fringe Packet Observations with the CHARA Array II omega Andromeda HD 178911 and xi Cephei The Astronomical Journal 148 3 48 arXiv 1407 0639 Bibcode 2014AJ 148 48F doi 10 1088 0004 6256 148 3 48 S2CID 12909818 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 a b Pourbaix D Tokovinin A A Batten A H Fekel F C Hartkopf W I et al 2004 SB9 The ninth catalogue of spectroscopic binary orbits Astronomy amp Astrophysics 424 2 727 732 arXiv astro ph 0406573 Bibcode 2004A amp A 424 727P doi 10 1051 0004 6361 20041213 S2CID 119387088 a b Naming Stars IAU org Retrieved 16 December 2017 Hessman F V Dhillon V S Winget D E Schreiber M R Horne K Marsh T R Guenther E Schwope A Heber U 2010 On the naming convention used for multiple star systems and extrasolar planets arXiv 1012 0707 astro ph SR Islamic Crescent Project Star names Archived from the original on 2008 02 02 Retrieved 2010 12 08 Allen R H 1963 Star Names Their Lore and Meaning Reprint ed New York Dover Publications Inc p 159 ISBN 0 486 21079 0 Retrieved 2010 12 12 IAU Working Group on Star Names WGSN International Astronomical Union retrieved 22 May 2016 WG Triennial Report 2015 2018 Star Names PDF p 5 Retrieved 2018 07 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 in Chinese 香港太空館 研究資源 亮星中英對照表 Archived January 29 2011 at the Wayback Machine Hong Kong Space Museum Accessed on line November 23 2010 Retrieved from https en wikipedia org w index php title Xi Cephei amp oldid 1170981674, wikipedia, wiki, book, books, library,

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