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N Scorpii

From Wikipedia, the free encyclopedia
Star in the constellation of Scorpius
N Scorpii
Location of N Scorpii on the map
Observation data
Epoch J2000      Equinox J2000
ConstellationScorpius
Right ascension16h 31m 22.93300s[1]
Declination−34° 42′ 15.7146″[1]
Apparent magnitude (V)4.23[2]
Characteristics
Spectral typeB2 III-IV[3]
U−Bcolor index−0.76[2]
B−Vcolor index−0.17[2]
Variable typecandidateβ Cephei[4]
Astrometry
Radial velocity (Rv)0.8±1.5[5] km/s
Proper motion (μ)RA: −12.05±0.20mas/yr[1]
Dec.: −18.16±0.13mas/yr[1]
Parallax (π)5.88±0.19 mas[1]
Distance550 ± 20 ly
(170 ± 5 pc)
Absolute magnitude (MV)−1.91[6]
Details
Mass7.8±0.1[7] M
Radius6.25[8] R
Luminosity (bolometric)6,918[9] L
Surface gravity (log g)4.0[9] cgs
Temperature21,877[9] K
Metallicity[Fe/H]+0.01[10] dex
Rotational velocity (v sin i)70±8[11] km/s
Age22±4[7] Myr
Other designations
N Scorpii,72 G. Scorpii[12],CD−34°11044,CPD−34°6528,FK5 1431,GC 22195,HD 148703,HIP 80911,HR 6143,SAO 207732[13]
Database references
SIMBADdata

N Scorpii, also known asHD 148703, is a solitary,[14] bluish-white huedstar located in the southernconstellationScorpius. It has anapparent magnitude of 4.23, making it readily visible to thenaked eye. N Scorpii was initially given theBayer designation Alpha Normae byLacaille but it was later moved fromNorma to Scorpius.[15] N Scorpii is currently located 550light years away based onparallax measurements from theHipparcos satellite and is part of the Upper Scorpius–Centaurus region of theScorpius–Centaurus association.[16]

N Scorpii has been given severalstellar classifications over the years. It has been given theluminosity class of amain sequence star (V),[17] asubgiant (IV),[18] an evolvedgiant star (III),[19] or a blend between the last two classes (III-IV).[3] It is generally classified as either a B2 or B3 star several times hotter than theSun. HD 148703 is a candidateβ Cephei variable[4] and its variability was first noticed in 1983 by C. Sterken.[20] Further observations were made by Abt et al. (2002) by observing itsprojected rotational velocity.[21] It was identified as a candidate in 2002 in a survey for non-radial pulsations inB-type stars.[22]

The object has two generally accepted classes: B2 III-IV and B2 IV. It has 7.8 times themass of the Sun[7] and 6.25 times itssize.[8] It has abolometric luminosity 6,918 times greater than the Sun from itsphotosphere at aneffective temperature of21,877 K.[9] N Scorpii is estimated to be 22million years old,[7] which is twice the average age of the aforementioned association. Like most hot stars, N Scorpii spins rapidly, having aprojected rotational velocity of70 km/s.[11]

References

[edit]
  1. ^abcdvan Leeuwen, Floor (13 August 2007)."Validation of the new Hipparcos reduction".Astronomy & Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.eISSN 1432-0746.ISSN 0004-6361. Hipparcos record for this source atVizieR.
  2. ^abcDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".VizieR Online Data Catalog.2237.Bibcode:2002yCat.2237....0D.
  3. ^abHouk, N. (1982).Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations −40° to −26°.Bibcode:1982mcts.book.....H.
  4. ^abStankov, Anamarija; Handler, Gerald (June 2005)."Catalog of Galactic β Cephei Stars".The Astrophysical Journal Supplement Series.158 (2):193–216.arXiv:astro-ph/0506495.Bibcode:2005ApJS..158..193S.doi:10.1086/429408.eISSN 1538-4365.ISSN 0067-0049.
  5. ^Gontcharov, G. A. (November 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.eISSN 1562-6873.ISSN 1063-7737.S2CID 119231169.
  6. ^Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.eISSN 1562-6873.ISSN 1063-7737.S2CID 119257644.
  7. ^abcdTetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (October 12, 2010)."A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun".Monthly Notices of the Royal Astronomical Society.410 (1). Oxford University Press (OUP):190–200.arXiv:1007.4883.Bibcode:2011MNRAS.410..190T.doi:10.1111/j.1365-2966.2010.17434.x.ISSN 0035-8711.
  8. ^abKervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022)."Stellar and substellar companions fromGaia EDR3".Astronomy & Astrophysics.657: A7.arXiv:2109.10912.Bibcode:2022A&A...657A...7K.doi:10.1051/0004-6361/202142146.eISSN 1432-0746.ISSN 0004-6361.
  9. ^abcdSartori, M. J.; Lépine, J. R. D.; Dias, W. S. (June 2003)."Formation scenarios for the young stellar associations between galactic longitudesl = 280° - 360°".Astronomy & Astrophysics.404 (3):913–926.arXiv:astro-ph/0304426.Bibcode:2003A&A...404..913S.doi:10.1051/0004-6361:20030581.eISSN 1432-0746.ISSN 0004-6361.
  10. ^Anders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia DR2 stars brighter thanG = 18".Astronomy & Astrophysics.628: A94.arXiv:1904.11302.Bibcode:2019A&A...628A..94A.doi:10.1051/0004-6361/201935765.eISSN 1432-0746.ISSN 0004-6361.
  11. ^abBrown, A. G. A.; Verschueren, W. (March 1997). "High S/N Echelle spectroscopy in young stellar groups. II. Rotational velocities of early-type stars in SCO OB2".Astronomy & Astrophysics.319:811–838.arXiv:astro-ph/9608089.Bibcode:1997A&A...319..811B.ISSN 0004-6361.
  12. ^Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas".Resultados del Observatorio Nacional Argentino.1.Bibcode:1879RNAO....1.....G.
  13. ^"N Scorpii".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedOctober 17, 2022.
  14. ^Eggleton, P. P.; Tokovinin, A. A. (11 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.eISSN 1365-2966.ISSN 0035-8711.
  15. ^"Norma Constellation (the Level): Stars, Story, Facts... | Constellation Guide".www.constellation-guide.com. Retrieved11 October 2021.
  16. ^Rizzuto, A. C.; Ireland, M. J.; Robertson, J. G. (18 August 2011)."Multidimensional Bayesian membership analysis of the Sco OB2 moving group".Monthly Notices of the Royal Astronomical Society.416 (4):3108–3117.arXiv:1106.2857.Bibcode:2011MNRAS.416.3108R.doi:10.1111/j.1365-2966.2011.19256.x.ISSN 0035-8711.
  17. ^de Vaucouleurs, A. (1 August 1957)."Spectral Types and Luminosities of B, A and F Southern Stars".Monthly Notices of the Royal Astronomical Society.117 (4):449–462.Bibcode:1957MNRAS.117..449D.doi:10.1093/mnras/117.4.449.eISSN 1365-2966.ISSN 0035-8711.
  18. ^Buscombe, W. (1 May 1969)."Line Strengths for Southern OB stars--II: Observations with Moderate Dispersion".Monthly Notices of the Royal Astronomical Society.144 (1):31–39.Bibcode:1969MNRAS.144...31B.doi:10.1093/mnras/144.1.31.ISSN 0035-8711.
  19. ^Hiltner, W. A.; Garrison, R. F.; Schild, R. E. (July 1969)."MK Spectral Types for Bright Southern OB Stars".The Astrophysical Journal.157: 313.Bibcode:1969ApJ...157..313H.doi:10.1086/150069.eISSN 1538-4357.ISSN 0004-637X.
  20. ^Sterken, C.; Jerzykiewicz, M. (1983). "Search for beta Cephei stars south of declination -20 II. Photometric and spectrographic observations of early B giants and subgiants - Winter objects".Acta Astronomica.33:89–111.Bibcode:1983AcA....33...89S.ISSN 0001-5237.
  21. ^Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002)."Rotational Velocities of B Stars".The Astrophysical Journal.573 (1):359–365.Bibcode:2002ApJ...573..359A.doi:10.1086/340590.ISSN 0004-637X.
  22. ^Schrijvers, C.; Telting, J. H.; De Ridder, J. (2002). "A Spectroscopic Search for Non-Radial Pulsations in Early B-Type Stars".IAU Colloq. 185: Radial and Nonradial Pulsationsn as Probes of Stellar Physics.259: 204.Bibcode:2002ASPC..259..204S.
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