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4 Camelopardalis

From Wikipedia, the free encyclopedia
Probable multiple star system in the constellation Camelopardalis
4 Camelopardalis
Observation data
Epoch J2000      Equinox J2000
ConstellationCamelopardalis
Right ascension04h 48m 00.2729s[1]
Declination+56° 45′ 25.837″[1]
Apparent magnitude (V)5.29[2]
Characteristics
Spectral typeA3m[3]
U−Bcolor index0.12[4]
B−Vcolor index0.246±0.003[2]
Astrometry
Radial velocity (Rv)+22.50±0.9[5] km/s
Proper motion (μ)RA: +52.892[1]mas/yr
Dec.: −140.618[1]mas/yr
Parallax (π)18.4464±0.1109 mas[1]
Distance177 ± 1 ly
(54.2 ± 0.3 pc)
Absolute magnitude (MV)1.68[2]
Orbit[6]
PrimaryAa
CompanionAb
Period (P)90yr
Semi-major axis (a)0.503″
Eccentricity (e)0.87
Inclination (i)120.0°
Longitude of the node (Ω)54.5°
Argument of periastron (ω)
(secondary)
235.9°
Details
Mass2.01[7] M
Radius2.57+0.05
−0.17
[8] R
Luminosity17.64[2] L
Surface gravity (log g)3.98[9] cgs
Temperature7,700[9] K
Metallicity [Fe/H]+0.27[9] dex
Rotational velocity (v sin i)75[10] km/s
Age560[7] Myr
Other designations
4 Cam,BD+56°973,FK5 175,HD 30121,HIP 22287,HR 1511,SAO 24829[11]
Database references
SIMBADdata

4 Camelopardalis is a probablemultiple star in the northernconstellation ofCamelopardalis,[11] located 177 light years away from the Sun, based upon parallax.[1] With a combinedapparent visual magnitude of 5.29,[2] it is visible to the naked eye as a faint, white-hued star. The pair have a relatively highproper motion, traversing thecelestial sphere at an angular rate of0.158 per year.[12] The system's proper motion makes it a candidate for membership in theIC 2391 supercluster.[13] They are moving away from the Earth with a heliocentricradial velocity of 22.5 km/s.[5]

The brighter member, designated component A, is classified as anAm star, which indicates that the spectrum shows abnormalities of certain elements.[14] It is an estimated 560[7] million years old and is spinning with aprojected rotational velocity of 75[10] The star has 2.01[7] times themass of the Sun and 2.57[8] times theSun's radius. It is radiating 18[2] times theSun's luminosity from itsphotosphere at aneffective temperature of 7,700 K.[9]

There is a faint, magnitude 9.49 companion at anangular separation of0.610″ – component B; the pair most likely form a binary systemwith a period of about 90 years.[6] There is also a 13th-magnitudevisual companion13 away which shares a common proper motion and parallax.[15][6] Another listed companion, a 12th-magnitude star nearly2 away, is probably unrelated.[16]

References

[edit]
  1. ^abcdefBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abcdefAnderson, 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. ^Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications",Astronomical Journal,74:375–406,Bibcode:1969AJ.....74..375C,doi:10.1086/110819
  4. ^Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data. SIMBAD,Bibcode:1986EgUBV........0M
  5. ^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,S2CID 119231169.
  6. ^abcTokovinin, Andrei; Everett, Mark E.; Horch, Elliott P.; Torres, Guillermo; Latham, David W. (2019), "Speckle Observations and Orbits of Multiple Stars",The Astronomical Journal,158 (4): 167,arXiv:1908.11445,Bibcode:2019AJ....158..167T,doi:10.3847/1538-3881/ab4137,S2CID 201698428.
  7. ^abcdDe Rosa, R. J.; et al. (2014), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc",Monthly Notices of the Royal Astronomical Society,437 (2):1216–1240,arXiv:1311.7141,Bibcode:2014MNRAS.437.1216D,doi:10.1093/mnras/stt1932.
  8. ^abBrown, 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.
  9. ^abcdTakeda, Yoichi; et al. (October 2018), "Photospheric carbon, nitrogen, and oxygen abundances of A-type main-sequence stars*",Publications of the Astronomical Society of Japan,70 (5): 91,arXiv:1807.06265,Bibcode:2018PASJ...70...91T,doi:10.1093/pasj/psy091, 91.
  10. ^abRoyer, F.; et al. (2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i in the northern hemisphere",Astronomy and Astrophysics,393 (3):897–911,arXiv:astro-ph/0205255,Bibcode:2002A&A...393..897R,doi:10.1051/0004-6361:20020943,S2CID 14070763
  11. ^ab"4 Cam",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2019-04-14.
  12. ^Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)",The Astronomical Journal,129 (3):1483–1522,arXiv:astro-ph/0412070,Bibcode:2005AJ....129.1483L,doi:10.1086/427854,S2CID 2603568.
  13. ^Eggen, Olin J. (December 1995), "Reality Tests of Superclusters in the Young Disk Population",Astronomical Journal,110: 2862,Bibcode:1995AJ....110.2862E,doi:10.1086/117734.
  14. ^Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars",Astronomy and Astrophysics,498 (3):961–966,Bibcode:2009A&A...498..961R,doi:10.1051/0004-6361/200810788
  15. ^Brown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  16. ^Brown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.

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