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WR 86

WR 86 is a visual binary in the constellation Scorpius consisting of a Wolf-Rayet star and a β Cephei variable. It lies 2° west of NGC 6357 on the edge of the Great Rift in the Milky Way in the tail of the Scorpion.

WR 86

A light curve for V1035 Scorpii, plotted from TESS data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Scorpius
Right ascension 17h 18m 23.06137s[2]
Declination −34° 24′ 30.6308″[2]
Apparent magnitude (V) 9.27[3]
Characteristics
Evolutionary stage Wolf-Rayet star
Spectral type WC7 + B0III[4]
Apparent magnitude (J) 7.436[5]
Apparent magnitude (K) 6.666[6]
U−B color index −0.07[7]
B−V color index +0.63[7]
Variable type β Cep[3]
Astrometry
Proper motion (μ) RA: −0.92[2] mas/yr
Dec.: −4.80[2] mas/yr
Parallax (π)1.84 ± 1.62 mas[2]
Distance2,100 ± 800[4] pc
Absolute magnitude (MV)−4.3 + −4.3[4]
Details
WR
Radius10[8] R
Luminosity200,000[4][8] L
Temperature56,000[8] K
B
Mass19 M
Radius~8.5 (SBL) R
Luminosity63,000[4] L
Temperature31,405[4] K
Age4.0[4] Myr
Other designations
V1035 Scorpii, CD−34°11622, HD 156327, HIP 84655, 2MASS J17182306-3424306, WDS J17184-3425
Database references
SIMBADdata

WR 86 is a binary with two components of equal visual brightness 0.3" apart.[9] One has the emission-line spectrum of a WC7 Wolf-Rayet star, while the other is a B0 giant. The blue giant varies slightly in brightness every 3.5 hours. The WR star may also be slightly variable.[4]

The pulsations of the B-type giant are characteristic of a β Cephei variable. Analysis of its pulsations and comparison to the expected properties of a WC7 star suggest that both stars could have evolved without mass exchange. The WR and B stars would have had initial masses of 40 M and 20 M respectively four million years ago.[4]

References edit

  1. ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. ^ a b c d e 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.
  3. ^ a b Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  4. ^ a b c d e f g h i Paardekooper, S. J.; Veen, P. M.; Van Genderen, A. M.; Van Der Hucht, K. A. (2002). "On the variability of the visual binary WR86. WC7 with a β-Cephei companion". Astronomy and Astrophysics. 384 (3): 1012. Bibcode:2002A&A...384.1012P. doi:10.1051/0004-6361:20020085.
  5. ^ Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". CDS/ADC Collection of Electronic Catalogues. 2246: II/246. Bibcode:2003yCat.2246....0C.
  6. ^ Van Der Hucht, K. A. (2006). "New Galactic Wolf-Rayet stars, and candidates. An annex to the VIIth Catalogue of Galactic Wolf-Rayet Stars". Astronomy and Astrophysics. 458 (2): 453–459. arXiv:astro-ph/0609008. Bibcode:2006A&A...458..453V. doi:10.1051/0004-6361:20065819. S2CID 119104786.
  7. ^ a b Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  8. ^ a b c Sander, A.; Hamann, W.-R.; Todt, H. (2012). "The Galactic WC stars. Stellar parameters from spectral analyses indicate a new evolutionary sequence". Astronomy & Astrophysics. 540: A144. arXiv:1201.6354. Bibcode:2012A&A...540A.144S. doi:10.1051/0004-6361/201117830. S2CID 119182468.
  9. ^ 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.

visual, binary, constellation, scorpius, consisting, wolf, rayet, star, cephei, variable, lies, west, 6357, edge, great, rift, milky, tail, scorpion, light, curve, v1035, scorpii, plotted, from, tess, data, observation, dataepoch, j2000, equinox, j2000, 0const. WR 86 is a visual binary in the constellation Scorpius consisting of a Wolf Rayet star and a b Cephei variable It lies 2 west of NGC 6357 on the edge of the Great Rift in the Milky Way in the tail of the Scorpion WR 86A light curve for V1035 Scorpii plotted from TESS data 1 Observation dataEpoch J2000 0 Equinox J2000 0Constellation ScorpiusRight ascension 17h 18m 23 06137s 2 Declination 34 24 30 6308 2 Apparent magnitude V 9 27 3 CharacteristicsEvolutionary stage Wolf Rayet starSpectral type WC7 B0III 4 Apparent magnitude J 7 436 5 Apparent magnitude K 6 666 6 U B color index 0 07 7 B V color index 0 63 7 Variable type b Cep 3 AstrometryProper motion m RA 0 92 2 mas yr Dec 4 80 2 mas yrParallax p 1 84 1 62 mas 2 Distance2 100 800 4 pcAbsolute magnitude MV 4 3 4 3 4 DetailsWRRadius10 8 R Luminosity200 000 4 8 L Temperature56 000 8 KBMass19 M Radius 8 5 SBL R Luminosity63 000 4 L Temperature31 405 4 KAge4 0 4 MyrOther designationsV1035 Scorpii CD 34 11622 HD 156327 HIP 84655 2MASS J17182306 3424306 WDS J17184 3425Database referencesSIMBADdataWR 86 is a binary with two components of equal visual brightness 0 3 apart 9 One has the emission line spectrum of a WC7 Wolf Rayet star while the other is a B0 giant The blue giant varies slightly in brightness every 3 5 hours The WR star may also be slightly variable 4 The pulsations of the B type giant are characteristic of a b Cephei variable Analysis of its pulsations and comparison to the expected properties of a WC7 star suggest that both stars could have evolved without mass exchange The WR and B stars would have had initial masses of 40 M and 20 M respectively four million years ago 4 References edit MAST Barbara A Mikulski Archive for Space Telescopes Space Telescope Science Institute Retrieved 8 December 2021 a b c d e 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 a b Samus N N Durlevich O V et al 2009 VizieR Online Data Catalog General Catalogue of Variable Stars Samus 2007 2013 VizieR On line Data Catalog B GCVS Originally Published in 2009yCat 102025S 1 Bibcode 2009yCat 102025S a b c d e f g h i Paardekooper S J Veen P M Van Genderen A M Van Der Hucht K A 2002 On the variability of the visual binary WR86 WC7 with a b Cephei companion Astronomy and Astrophysics 384 3 1012 Bibcode 2002A amp A 384 1012P doi 10 1051 0004 6361 20020085 Cutri Roc M Skrutskie Michael F Van Dyk Schuyler D Beichman Charles A Carpenter John M Chester Thomas Cambresy Laurent Evans Tracey E Fowler John W Gizis John E Howard Elizabeth V Huchra John P Jarrett Thomas H Kopan Eugene L Kirkpatrick J Davy Light Robert M Marsh Kenneth A McCallon Howard L Schneider Stephen E Stiening Rae Sykes Matthew J Weinberg Martin D Wheaton William A Wheelock Sherry L Zacarias N 2003 VizieR Online Data Catalog 2MASS All Sky Catalog of Point Sources Cutri 2003 CDS ADC Collection of Electronic Catalogues 2246 II 246 Bibcode 2003yCat 2246 0C Van Der Hucht K A 2006 New Galactic Wolf Rayet stars and candidates An annex to the VIIth Catalogue of Galactic Wolf Rayet Stars Astronomy and Astrophysics 458 2 453 459 arXiv astro ph 0609008 Bibcode 2006A amp A 458 453V doi 10 1051 0004 6361 20065819 S2CID 119104786 a b Ducati J R 2002 VizieR Online Data Catalog Catalogue of Stellar Photometry in Johnson s 11 color system CDS ADC Collection of Electronic Catalogues 2237 Bibcode 2002yCat 2237 0D a b c Sander A Hamann W R Todt H 2012 The Galactic WC stars Stellar parameters from spectral analyses indicate a new evolutionary sequence Astronomy amp Astrophysics 540 A144 arXiv 1201 6354 Bibcode 2012A amp A 540A 144S doi 10 1051 0004 6361 201117830 S2CID 119182468 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 Retrieved from https en wikipedia org w index php title WR 86 amp oldid 1154747657, wikipedia, wiki, book, books, library,

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