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Omega1 Cygni

From Wikipedia, the free encyclopedia
B-type subgiant star in the constellation Cygnus
For other stars with this Bayer designation, seeω Cygni.
Omega1 Cygni
Location of ω1 Cygni (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCygnus
Right ascension20h 30m 03.54116s[1]
Declination+48° 57′ 05.6446″[1]
Apparent magnitude (V)+4.93 - 4.96[2]
Characteristics
Spectral typeB2.5 IV[3]
U−Bcolor index−0.68[4]
B−Vcolor index−0.09[4]
Variable typeβ Cep[5](λ Eri[2])
Astrometry
Radial velocity (Rv)−21.9±2.0[6] km/s
Proper motion (μ)RA: +10.883[7]mas/yr
Dec.: +7.057[7]mas/yr
Parallax (π)2.5878±0.1637 mas[7]
Distance1,260 ± 80 ly
(390 ± 20 pc)
Absolute magnitude (MV)−2.65[8]
Details
Mass8.1±0.2[3] M
Radius4.55[9][a] R
Luminosity1,549[9] L
Surface gravity (log g)2.312[10] cgs
Temperature16,982[9] K
Metallicity[Fe/H]0.0[8] dex
Rotational velocity (v sin i)145[11] km/s
Age33.2±4.5[3] Myr
Other designations
ω1 Cyg,45 Cygni,BD+48°3142,FK5 3641,HD 195556,HIP 101138,HR 7844,SAO 49712,V2014 Cygni[12]
Database references
SIMBADdata

Omega1 Cygni,Latinized fromω1 Cygni, is theBayer designation for a solitary[13]star in the northernconstellation ofCygnus. It is visible to the naked eye with anapparent visual magnitude of 4.94.[4] Based upon an annualparallax shift of2.59 mas,[7] it is estimated to lie roughly1,260 light years from theSun. Relative to its neighbors, this star has apeculiar velocity of25.7±2.2 km/s.[6]

Alight curve for V2014 Cygni, plotted fromTESS data[14]

This is a somewhatevolvedB-typesubgiant star with astellar classification of B2.5 IV.[3] Telting and colleagues report it as aBeta Cephei variable with a high degree of confidence as they found regular pulsations in itsspectrum in a high-resolution spectroscopy study published in 2006.[5] Its brightness varies irregularly by 0.034 magnitude every 1.137 days.[15]

Notes

[edit]
  1. ^Calculated, using theStefan-Boltzmann law and the star'seffective temperature and luminosity, with respect to thesolar nominal effective temperature of5,772 K:(5,77216,982)41.549=4.55 R.{\displaystyle {\sqrt {{\biggl (}{\frac {5,772}{16,982}}{\biggr )}^{4}\cdot 1.549}}=4.55\ R_{\odot }.}

References

[edit]
  1. ^abvan 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.
  2. ^ab"V2014 Cygni",International Variable Star Index, retrieved2020-09-02
  3. ^abcdTetzlaff, N.; et al. (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.
  4. ^abcMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  5. ^abTelting, J. H.; et al. (June 2006), "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars",Astronomy and Astrophysics,452 (3):945–953,Bibcode:2006A&A...452..945T,doi:10.1051/0004-6361:20054730,hdl:2066/36162.
  6. ^abBobylev, V. V.; Bajkova, A. T. (August 2013), "Galactic kinematics from a sample of young massive stars",Astronomy Letters,39 (8):532–549,arXiv:1307.1677,Bibcode:2013AstL...39..532B,doi:10.1134/S106377371308001X,S2CID 118568203.
  7. ^abcdBrown, 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 atVizieR.
  8. ^abGontcharov, G. A. (2012), "Dependence of kinematics on the age of stars in the solar neighborhood",Astronomy Letters,38 (12):771–782,arXiv:1606.08814,Bibcode:2012AstL...38..771G,doi:10.1134/S1063773712120031,S2CID 118345778.
  9. ^abcSimón-Díaz, S.; Godart, M.; Castro, N.; Herrero, A.; Aerts, C.; Puls, J.; Telting, J.; Grassitelli, L. (2017), "The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars",Astronomy and Astrophysics,597: A22,arXiv:1608.05508,Bibcode:2017A&A...597A..22S,doi:10.1051/0004-6361/201628541,S2CID 3478126.
  10. ^McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017), "Fundamental parameters and infrared excesses of Tycho–Gaia stars",Monthly Notices of the Royal Astronomical Society,471 (1):770–791,arXiv:1706.02208,Bibcode:2017MNRAS.471..770M,doi:10.1093/mnras/stx1433,S2CID 73594365.
  11. ^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.
  12. ^"* ome01 Cyg -- Pulsating variable Star".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-02-22.
  13. ^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.
  14. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved27 November 2022.
  15. ^Lefèvre, L.; et al. (2009), "A systematic study of variability among OB-stars based on HIPPARCOS photometry",Astronomy and Astrophysics,507 (2): 1141,Bibcode:2009A&A...507.1141L,doi:10.1051/0004-6361/200912304.
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