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HR 6875

HR 6875, previously known as Sigma Telescopii, is a single[10] star in the constellation Corona Australis. It has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.24.[2] This object is located at a distance of approximately 550 light years from the Sun based on parallax.[1] It is listed as a member of the Sco OB2 association.[7]

HR 6875
Observation data
Epoch J2000      Equinox J2000
Constellation Corona Australis
Right ascension 18h 24m 18.24148s[1]
Declination −44° 06′ 36.9008″[1]
Apparent magnitude (V) 5.24[2]
Characteristics
Spectral type B3 V[3]
B−V color index −0.163±0.004[2]
Astrometry
Radial velocity (Rv)+0.00±7.40[2] km/s
Proper motion (μ) RA: −2.949[1] mas/yr
Dec.: −23.107[1] mas/yr
Parallax (π)5.9327 ± 0.2341 mas[1]
Distance550 ± 20 ly
(169 ± 7 pc)
Absolute magnitude (MV)−0.63[2]
Details
Mass6.2±0.1[4] M
Radius3.9[5] R
Luminosity (bolometric)1,098[6] L
Temperature20,350[6] K
Rotational velocity (v sin i)248±12[7] km/s
Age103[8] Myr
Other designations
CD−44° 12569, FK5 3461, HD 168905, HIP 90200, HR 6875, SAO 228982, WDS J18243-4407A[9]
Database references
SIMBADdata

This is a hot B-type main-sequence star with a stellar classification of B3 V.[3] It is around 103[8] million years old and is spinning rapidly with a projected rotational velocity of 248 km/s or perhaps higher.[7] The star has six[4] times the mass of the Sun and about four[5] times the Sun's radius. It is radiating more than a thousand[6] times the luminosity of the Sun from its photosphere at an effective temperature of 20,350 K.[6]

A magnitude 10.13 visual companion is located at an angular separation of 74 along a position angle of 162°.[11]

References

  1. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b c d e 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 Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
  4. ^ a b Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
  5. ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics (Third ed.), 367 (2): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
  6. ^ a b c d Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483.
  7. ^ a b c Brown, A. G. A.; Verschueren, W. (1997), "High S/N Echelle spectroscopy in young stellar groups. II. Rotational velocities of early-type stars in SCO OB2", Astronomy and Astrophysics, 319: 811, arXiv:astro-ph/9608089, Bibcode:1997A&A...319..811B.
  8. ^ a b Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.
  9. ^ "HD 168905". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-14.
  10. ^ 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.
  11. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ....122.3466M, doi:10.1086/323920, retrieved 2015-07-22

6875, previously, known, sigma, telescopii, single, star, constellation, corona, australis, blue, white, dimly, visible, naked, with, apparent, visual, magnitude, this, object, located, distance, approximately, light, years, from, based, parallax, listed, memb. HR 6875 previously known as Sigma Telescopii is a single 10 star in the constellation Corona Australis It has a blue white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5 24 2 This object is located at a distance of approximately 550 light years from the Sun based on parallax 1 It is listed as a member of the Sco OB2 association 7 HR 6875 Observation dataEpoch J2000 Equinox J2000Constellation Corona AustralisRight ascension 18h 24m 18 24148s 1 Declination 44 06 36 9008 1 Apparent magnitude V 5 24 2 CharacteristicsSpectral type B3 V 3 B V color index 0 163 0 004 2 AstrometryRadial velocity Rv 0 00 7 40 2 km sProper motion m RA 2 949 1 mas yr Dec 23 107 1 mas yrParallax p 5 9327 0 2341 mas 1 Distance550 20 ly 169 7 pc Absolute magnitude MV 0 63 2 DetailsMass6 2 0 1 4 M Radius3 9 5 R Luminosity bolometric 1 098 6 L Temperature20 350 6 KRotational velocity v sin i 248 12 7 km sAge103 8 MyrOther designationsCD 44 12569 FK5 3461 HD 168905 HIP 90200 HR 6875 SAO 228982 WDS J18243 4407A 9 Database referencesSIMBADdataThis is a hot B type main sequence star with a stellar classification of B3 V 3 It is around 103 8 million years old and is spinning rapidly with a projected rotational velocity of 248 km s or perhaps higher 7 The star has six 4 times the mass of the Sun and about four 5 times the Sun s radius It is radiating more than a thousand 6 times the luminosity of the Sun from its photosphere at an effective temperature of 20 350 K 6 A magnitude 10 13 visual companion is located at an angular separation of 74 along a position angle of 162 11 References Edit a b c d e f Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c d e 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 Houk Nancy 1978 Michigan catalogue of two dimensional spectral types for the HD stars vol 2 Ann Arbor Dept of Astronomy University of Michigan Bibcode 1978mcts book H a b Tetzlaff N Neuhauser R Hohle M M January 2011 A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun Monthly Notices of the Royal Astronomical Society 410 1 190 200 arXiv 1007 4883 Bibcode 2011MNRAS 410 190T doi 10 1111 j 1365 2966 2010 17434 x S2CID 118629873 a b Pasinetti Fracassini L E et al February 2001 Catalogue of Apparent Diameters and Absolute Radii of Stars CADARS Astronomy and Astrophysics Third ed 367 2 521 524 arXiv astro ph 0012289 Bibcode 2001A amp A 367 521P doi 10 1051 0004 6361 20000451 S2CID 425754 a b c d Hohle M M et al April 2010 Masses and luminosities of O and B type stars and red supergiants Astronomische Nachrichten 331 4 349 arXiv 1003 2335 Bibcode 2010AN 331 349H doi 10 1002 asna 200911355 S2CID 111387483 a b c Brown A G A Verschueren W 1997 High S N Echelle spectroscopy in young stellar groups II Rotational velocities of early type stars in SCO OB2 Astronomy and Astrophysics 319 811 arXiv astro ph 9608089 Bibcode 1997A amp A 319 811B a b Gontcharov G A November 2012 Spatial distribution and kinematics of OB stars Astronomy Letters 38 11 694 706 arXiv 1606 09028 Bibcode 2012AstL 38 694G doi 10 1134 S1063773712110035 S2CID 119108982 HD 168905 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2018 07 14 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 B D et al 2014 The Washington Visual Double Star Catalog The Astronomical Journal 122 6 3466 Bibcode 2001AJ 122 3466M doi 10 1086 323920 retrieved 2015 07 22 Retrieved from https en wikipedia org w index php title HR 6875 amp oldid 1124783270, wikipedia, wiki, book, books, library,

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