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12 Lyncis

12 Lyncis, abbreviated 12 Lyn, is a triple star[8] system in the constellation Lynx. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.87. When seen through a telescope, it can be separated into three stars: two components with magnitudes 5.4 and 6.0 that lie at an angular separation by 1.8 (as of 1992) and a yellow-hued star of magnitude 7.2 at a separation of 8.6″ (as of 1990).[9][10] The orbit of the two brighter stars is not known with certainty, but appears to have a period of somewhere around 700 to 900 years.[11] The pair have a projected separation of 128 AU.[4] Parallax indicates the system is 210±10 light years distant from Earth.[1]

12 Lyn
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 06h 46m 14.13019s[1]
Declination +59° 26′ 30.0227″[1]
Apparent magnitude (V) 4.86[2] (5.44 / 6.00)[3]
Characteristics
Spectral type A3V[2] (A1.5V + A2V)[4]
U−B color index +0.08[5]
B−V color index +0.084±0.012[2]
Astrometry
Radial velocity (Rv)−3.0±4.2[6] km/s
Proper motion (μ) RA: −19.63[1] mas/yr
Dec.: −7.23[1] mas/yr
Parallax (π)15.19 ± 0.78 mas[1]
Distance210 ± 10 ly
(66 ± 3 pc)
Absolute magnitude (MV)0.77[2]
Orbit[3]
Period (P)907.6 yr
Semi-major axis (a)2.30″
Eccentricity (e)0.3700
Inclination (i)134.7°
Longitude of the node (Ω)166.5°
Periastron epoch (T)B 2677.4
Argument of periastron (ω)
(secondary)
322.6°
Details
12 Lyn A
Radius2.52[4] R
Rotational velocity (v sin i)90±30[4] km/s
12 Lyn B
Radius2.44[4] R
Rotational velocity (v sin i)100±30[4] km/s
Other designations
12 Lyn, BD+59°1015, GC 9850, HD 48250, HIP 32438, HR 2470, SAO 25939, WDS 06462+5927[7]
Database references
SIMBAD12 Lyn
12 Lyn A
12 Lyn B

References edit

  1. ^ a b c d e f van Leeuwen, F.; et al. (2007). . Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Archived from the original on 2016-04-02.
  2. ^ a b c d 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.
  3. ^ a b . United States Naval Observatory. Archived from the original on 1 August 2017. Retrieved 28 May 2017.
  4. ^ a b c d e f Howe, K. S.; Clarke, C. J. (January 2009). "An analysis of v sin (i) correlations in early-type binaries". Monthly Notices of the Royal Astronomical Society. 392 (1): 448–454. Bibcode:2009MNRAS.392..448H. doi:10.1111/j.1365-2966.2008.14073.x.
  5. ^ Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode:1966CoLPL...4...99J.
  6. ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 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.
  7. ^ "* 12 Lyn". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 20 November 2012.
  8. ^ 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.
  9. ^ Mason, Brian D.; et al. (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.
  10. ^ Monks, Neale (2010). Go-To Telescopes Under Suburban Skies. New York, New York: Springer Science & Business Media. p. 56. ISBN 9781441968517.
  11. ^ Malkov, O. Yu.; Tamazian, V.S.; Docobo, J.A.; Chulkov, D.A. (2012). "Dynamical Masses of a Selected Sample of Orbital Binaries". Astronomy and Astrophysics. 546: 5. Bibcode:2012A&A...546A..69M. doi:10.1051/0004-6361/201219774. A69.

lyncis, abbreviated, triple, star, system, constellation, lynx, visible, naked, faint, point, light, with, combined, apparent, visual, magnitude, when, seen, through, telescope, separated, into, three, stars, components, with, magnitudes, that, angular, separa. 12 Lyncis abbreviated 12 Lyn is a triple star 8 system in the constellation Lynx It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4 87 When seen through a telescope it can be separated into three stars two components with magnitudes 5 4 and 6 0 that lie at an angular separation by 1 8 as of 1992 and a yellow hued star of magnitude 7 2 at a separation of 8 6 as of 1990 9 10 The orbit of the two brighter stars is not known with certainty but appears to have a period of somewhere around 700 to 900 years 11 The pair have a projected separation of 128 AU 4 Parallax indicates the system is 210 10 light years distant from Earth 1 12 Lyn Observation dataEpoch J2000 Equinox J2000 Constellation Lynx Right ascension 06h 46m 14 13019s 1 Declination 59 26 30 0227 1 Apparent magnitude V 4 86 2 5 44 6 00 3 Characteristics Spectral type A3V 2 A1 5V A2V 4 U B color index 0 08 5 B V color index 0 084 0 012 2 AstrometryRadial velocity Rv 3 0 4 2 6 km sProper motion m RA 19 63 1 mas yr Dec 7 23 1 mas yrParallax p 15 19 0 78 mas 1 Distance210 10 ly 66 3 pc Absolute magnitude MV 0 77 2 Orbit 3 Period P 907 6 yrSemi major axis a 2 30 Eccentricity e 0 3700Inclination i 134 7 Longitude of the node W 166 5 Periastron epoch T B 2677 4Argument of periastron w secondary 322 6 Details12 Lyn ARadius2 52 4 R Rotational velocity v sin i 90 30 4 km s12 Lyn BRadius2 44 4 R Rotational velocity v sin i 100 30 4 km s Other designations12 Lyn BD 59 1015 GC 9850 HD 48250 HIP 32438 HR 2470 SAO 25939 WDS 06462 5927 7 Database referencesSIMBAD12 Lyn12 Lyn A12 Lyn BReferences edit a b c d e f van Leeuwen F et al 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 Archived from the original on 2016 04 02 a b c d 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 Sixth Catalog of Orbits of Visual Binary Stars United States Naval Observatory Archived from the original on 1 August 2017 Retrieved 28 May 2017 a b c d e f Howe K S Clarke C J January 2009 An analysis of v sin i correlations in early type binaries Monthly Notices of the Royal Astronomical Society 392 1 448 454 Bibcode 2009MNRAS 392 448H doi 10 1111 j 1365 2966 2008 14073 x Johnson H L 1966 UBVRIJKL Photometry of the Bright Stars Communications of the Lunar and Planetary Laboratory 4 99 Bibcode 1966CoLPL 4 99J Gontcharov G A 2006 Pulkovo Compilation of Radial Velocities for 35 495 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 12 Lyn SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 20 November 2012 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 Mason Brian D et al 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 Monks Neale 2010 Go To Telescopes Under Suburban Skies New York New York Springer Science amp Business Media p 56 ISBN 9781441968517 Malkov O Yu Tamazian V S Docobo J A Chulkov D A 2012 Dynamical Masses of a Selected Sample of Orbital Binaries Astronomy and Astrophysics 546 5 Bibcode 2012A amp A 546A 69M doi 10 1051 0004 6361 201219774 A69 Retrieved from https en wikipedia org w index php title 12 Lyncis amp oldid 1158502770, wikipedia, wiki, book, books, library,

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