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HD 31134

From Wikipedia, the free encyclopedia
Star in the constellation of Camelopardalis
HD 31134
Location of HD 31134 on the map (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCamelopardalis[1]
Right ascension04h 56m 07.07238s[2]
Declination+52° 52′ 11.0544″[2]
Apparent magnitude (V)5.74±0.01[3]
Characteristics
Evolutionary stagemain sequence[4]
Spectral typeA2 Vs[5] or A1 Vp[6]
U−Bcolor index+0.11[3]
B−Vcolor index+0.09[3]
Astrometry
Radial velocity (Rv)−15.1±2.5[7] km/s
Proper motion (μ)RA: −3.418mas/yr[2]
Dec.: +14.954mas/yr[2]
Parallax (π)6.8897±0.1144 mas[2]
Distance473 ± 8 ly
(145 ± 2 pc)
Absolute magnitude (MV)+0.19[1]
Details
Mass2.74±0.05[4] M
Radius4.38±0.22[8] R
Luminosity103+13
−11
[4] L
Surface gravity (log g)3.85[9] cgs
Temperature8,690[9] K
Metallicity[Fe/H]−0.11[10] dex
Rotational velocity (v sin i)60±1[11] km/s
Age432[12] Myr
Other designations
AG+52°472,BD+52°898,GC 5988,HD 31134,HIP 22936,HR 1561,SAO 24919[13]
Database references
SIMBADdata

HD 31134, also designated asHR 1561, is a solitarystar[14] located in the northerncircumpolar constellationCamelopardalis, the giraffe. It is faintly visible to thenaked eye as a white-hued star with anapparent magnitude of 5.74.[3]Gaia DR3parallax measurements place it 473light years away.[2] It appears to be approaching theSolar System with a heliocentricradial velocity of−15.1 km/s.[7] At its current distance, HD 31134's brightness is diminished by 0.35magnitudes due tointerstellar dust.[15] It has anabsolute magnitude of +0.19.[1]

The object has astellar classification of A2 Vs,[5] indicating that it is anA-type main-sequence star with sharp or narrowabsorption lines due to slow rotation. Two sources remove thes prefix and instead list it as an ordinary dwarf star[16][17] while one lists it as a moreevolvedgiant star.[18] Abt and Morell (1995) list it as a slightly hotter peculiarAp star,[6] but it is now considered unlikely to be chemically peculiar.[19] It has 2.74 times themass of the Sun and an enlargedradius of 4.38 R.[8] It radiates 103 times theluminosity of the Sun[4] from itsphotosphere at aneffective temperature of8,690 K.[9] HD 31134 is a rather evolved star, having completed 97.6% of itsmain sequence lifetime[4] at the age of 432million years.[12] Consistent with its spectrum, it spins modestly with aprojected rotational velocity of60 km/s.[11]

References

[edit]
  1. ^abcAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdOja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI".Astronomy and Astrophysics Supplement Series.89: 415.Bibcode:1991A&AS...89..415O.ISSN 0365-0138.
  4. ^abcdeZorec, J.; Royer, F. (January 2012)."Rotational velocities of A-type stars IV: Evolution of rotational velocities".Astronomy & Astrophysics.537: A120.arXiv:1201.2052.Bibcode:2012A&A...537A.120Z.doi:10.1051/0004-6361/201117691.eISSN 1432-0746.ISSN 0004-6361.S2CID 55586789.
  5. ^abCowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (April 1969)."A study of the bright stars. I. A catalogue of spectral classifications".The Astronomical Journal.74: 375.Bibcode:1969AJ.....74..375C.doi:10.1086/110819.ISSN 0004-6256.
  6. ^abAbt, Helmut A.; Morrell, Nidia I. (July 1995)."The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars".The Astrophysical Journal Supplement Series.99: 135.Bibcode:1995ApJS...99..135A.doi:10.1086/192182.ISSN 0067-0049.
  7. ^abGontcharov, 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.
  8. ^abKervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004)."The angular sizes of dwarf stars and subgiants".Astronomy & Astrophysics.426 (1):297–307.arXiv:astro-ph/0404180.Bibcode:2004A&A...426..297K.doi:10.1051/0004-6361:20035930.eISSN 1432-0746.ISSN 0004-6361.
  9. ^abcPhilip, A. G. D.; Egret, D. (May 1980). "An analysis of the Hauck-Mermillod catalogue of homogeneous four-color data. II".Astronomy and Astrophysics Supplement Series.40:199–205.Bibcode:1980A&AS...40..199P.ISSN 0365-0138.
  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. ^abRoyer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. (October 2002)."Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i".Astronomy & Astrophysics.393 (3):897–911.arXiv:astro-ph/0205255.Bibcode:2002A&A...393..897R.doi:10.1051/0004-6361:20020943.eISSN 1432-0746.ISSN 0004-6361.
  12. ^abGontcharov, G. A. (December 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.eISSN 1562-6873.ISSN 1063-7737.
  13. ^"HR 1561".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedJanuary 3, 2023.
  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.S2CID 14878976.
  15. ^Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017)."Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars".Monthly Notices of the Royal Astronomical Society.472 (4):3805–3820.arXiv:1709.01160.Bibcode:2017MNRAS.472.3805G.doi:10.1093/mnras/stx2219.eISSN 1365-2966.ISSN 0035-8711.
  16. ^Appenzeller, Immo (April 1967)."MK Spectral Types for 185 Bright Stars".Publications of the Astronomical Society of the Pacific.79 (467): 102.Bibcode:1967PASP...79..102A.doi:10.1086/128449.eISSN 1538-3873.ISSN 0004-6280.
  17. ^Cucchiaro, A.; Macau-Hercot, D.; Jaschek, M.; Jaschek, C. (July 1978). "Spectral classification from the ultraviolet line features of S2/68 spectra. III. Early A-type stars".Astronomy and Astrophysics Supplement Series.33:15–26.Bibcode:1978A&AS...33...15C.ISSN 0365-0138.
  18. ^Palmer, D. R.; Walker, E. N.; Jones, D. H. P.; Wallis, R. E. (1968). "The radial velocities spectral types and projected rotational velocities of 633 bright northern A stars".Royal Greenwich Observatory Bulletins.135: 385.Bibcode:1968RGOB..135..385P.
  19. ^Renson, P.; Manfroid, J. (19 March 2009)."Catalogue of Ap, HgMn and Am stars".Astronomy & Astrophysics.498 (3):961–966.Bibcode:2009A&A...498..961R.doi:10.1051/0004-6361/200810788.eISSN 1432-0746.ISSN 0004-6361.
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