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16 Persei
Location of 16 Persei (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Perseus
Right ascension 02h 50m 35.05979s [1]
Declination 38° 19′ 07.1080″ [1]
Apparent magnitude (V) 4.22 [2]
Characteristics
Spectral type F2III [3]
U−B color index +0.08 [4]
B−V color index +0.34 [4]
Variable type δ Sct(?) [5] [6]
Astrometry
Radial velocity (Rv)+14.00 [7] km/s
Proper motion (μ) RA: +195.77 [1]  mas/ yr
Dec.: −109.98 [1]  mas/ yr
Parallax (π)27.01 ± 0.19  mas [1]
Distance120.8 ± 0.8  ly
(37.0 ± 0.3  pc)
Absolute magnitude (MV)1.38 [2]
Details
Mass1.80 [8]  M☉
Radius3.2 [9]  R☉
Luminosity23.36 [2]  L☉
Surface gravity (log g)3.72 [10]  cgs
Temperature7,004 [10]  K
Metallicity [Fe/H]−0.04 [2]  dex
Rotational velocity (v sin i)149 [3] km/s
Age1.44 [8]  Gyr
Other designations
16 Per, NSV 956, BD+37°646, FK5 2194, GC 3401, HD 17584, HIP 13254, HR 840, SAO 55928, CCDM J02506+3818A, LTT 10924 [11]
Database references
SIMBAD data

16 Persei is a single, [12] suspected variable star [6] in the northern constellation of Perseus, located approximately 121 light years away based on parallax. [1] It is visible to the naked eye as a yellow-white hued star with an apparent visual magnitude of 4.22. [2] This object is moving further from the Earth with a heliocentric radial velocity of +14 km/s. [7] It displays a relatively high proper motion, traversing the celestial sphere at the rate of 0.224 ″ per year. [13]

Based upon a stellar classification of F2 III, [3] this matches an aging giant star that has exhausted the hydrogen at its core and is evolving away from the main sequence. It is a possible pulsating Delta Scuti variable, although there is some uncertainty about this classification. [6] However, Kunzli and North (1998) found no variation. [14] The star is 1.44 [8] billion years old with 1.8 [8] times the mass of the Sun and 3.2 [9] times the Sun's radius. It shows a high rotation rate with a projected rotational velocity of 149 km/s, [3] which is causing an equatorial bulge that is an estimated 24% larger than the polar radius. [15] 16 Persei is radiating 23 [2] times the Sun's luminosity from its photosphere at an effective temperature of 7,004 K. [10]

It has two reported visual companions: B, with magnitude 12.8 and separation 76.7", and C, with magnitude 10.43 and separation 234". [16]

References

  1. ^ a b c d e f Van 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. Vizier catalog entry
  2. ^ a b c d e f 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. Vizier catalog entry
  3. ^ a b c d Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050. Bibcode: 1995yCat.5050....0H.
  4. ^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42: 443. Bibcode: 2014JAVSO..42..443M. Vizier catalog entry
  5. ^ "NSV 956". The International Variable Star Index. AAVSO – American Association of Variable Star Observers. Retrieved 17 February 2019.
  6. ^ a b c Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. S2CID  125853869.
  7. ^ a b Wilson, R. E. (1953). General Catalogue of Stellar Radial Velocities. Carnegie Institution for Science. Bibcode: 1953GCRV..C......0W. LCCN  54001336.
  8. ^ a b c d Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.
  9. ^ a b Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv: astro-ph/9911002. Bibcode: 1999A&A...352..555A. Vizier catalog entry
  10. ^ a b c David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv: 1501.03154. Bibcode: 2015ApJ...804..146D. doi: 10.1088/0004-637X/804/2/146. S2CID  33401607. Vizier catalog entry
  11. ^ "16 Per". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-01.
  12. ^ 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.
  13. ^ 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.
  14. ^ Kunzli, M.; North, P. (January 1998). "Are metallic A-F giants evolved AM stars? Rotation and rate of binaries among giant F stars". Astronomy and Astrophysics Supplement. 127 (2): 277–294. arXiv: astro-ph/9710226. Bibcode: 1998A&AS..127..277K. doi: 10.1051/aas:1998350. S2CID  7535170.
  15. ^ van Belle, Gerard T. (March 2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20 (1): 51, arXiv: 1204.2572, Bibcode: 2012A&ARv..20...51V, doi: 10.1007/s00159-012-0051-2, S2CID  119273474.
  16. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. Vizier catalog entry
Retrieved from " https://en.wikipedia.org/?title=16_Persei&oldid=1079512013"
From Wikipedia, the free encyclopedia
16 Persei
Location of 16 Persei (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Perseus
Right ascension 02h 50m 35.05979s [1]
Declination 38° 19′ 07.1080″ [1]
Apparent magnitude (V) 4.22 [2]
Characteristics
Spectral type F2III [3]
U−B color index +0.08 [4]
B−V color index +0.34 [4]
Variable type δ Sct(?) [5] [6]
Astrometry
Radial velocity (Rv)+14.00 [7] km/s
Proper motion (μ) RA: +195.77 [1]  mas/ yr
Dec.: −109.98 [1]  mas/ yr
Parallax (π)27.01 ± 0.19  mas [1]
Distance120.8 ± 0.8  ly
(37.0 ± 0.3  pc)
Absolute magnitude (MV)1.38 [2]
Details
Mass1.80 [8]  M☉
Radius3.2 [9]  R☉
Luminosity23.36 [2]  L☉
Surface gravity (log g)3.72 [10]  cgs
Temperature7,004 [10]  K
Metallicity [Fe/H]−0.04 [2]  dex
Rotational velocity (v sin i)149 [3] km/s
Age1.44 [8]  Gyr
Other designations
16 Per, NSV 956, BD+37°646, FK5 2194, GC 3401, HD 17584, HIP 13254, HR 840, SAO 55928, CCDM J02506+3818A, LTT 10924 [11]
Database references
SIMBAD data

16 Persei is a single, [12] suspected variable star [6] in the northern constellation of Perseus, located approximately 121 light years away based on parallax. [1] It is visible to the naked eye as a yellow-white hued star with an apparent visual magnitude of 4.22. [2] This object is moving further from the Earth with a heliocentric radial velocity of +14 km/s. [7] It displays a relatively high proper motion, traversing the celestial sphere at the rate of 0.224 ″ per year. [13]

Based upon a stellar classification of F2 III, [3] this matches an aging giant star that has exhausted the hydrogen at its core and is evolving away from the main sequence. It is a possible pulsating Delta Scuti variable, although there is some uncertainty about this classification. [6] However, Kunzli and North (1998) found no variation. [14] The star is 1.44 [8] billion years old with 1.8 [8] times the mass of the Sun and 3.2 [9] times the Sun's radius. It shows a high rotation rate with a projected rotational velocity of 149 km/s, [3] which is causing an equatorial bulge that is an estimated 24% larger than the polar radius. [15] 16 Persei is radiating 23 [2] times the Sun's luminosity from its photosphere at an effective temperature of 7,004 K. [10]

It has two reported visual companions: B, with magnitude 12.8 and separation 76.7", and C, with magnitude 10.43 and separation 234". [16]

References

  1. ^ a b c d e f Van 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. Vizier catalog entry
  2. ^ a b c d e f 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. Vizier catalog entry
  3. ^ a b c d Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050. Bibcode: 1995yCat.5050....0H.
  4. ^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42: 443. Bibcode: 2014JAVSO..42..443M. Vizier catalog entry
  5. ^ "NSV 956". The International Variable Star Index. AAVSO – American Association of Variable Star Observers. Retrieved 17 February 2019.
  6. ^ a b c Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. S2CID  125853869.
  7. ^ a b Wilson, R. E. (1953). General Catalogue of Stellar Radial Velocities. Carnegie Institution for Science. Bibcode: 1953GCRV..C......0W. LCCN  54001336.
  8. ^ a b c d Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.
  9. ^ a b Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv: astro-ph/9911002. Bibcode: 1999A&A...352..555A. Vizier catalog entry
  10. ^ a b c David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv: 1501.03154. Bibcode: 2015ApJ...804..146D. doi: 10.1088/0004-637X/804/2/146. S2CID  33401607. Vizier catalog entry
  11. ^ "16 Per". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-01.
  12. ^ 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.
  13. ^ 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.
  14. ^ Kunzli, M.; North, P. (January 1998). "Are metallic A-F giants evolved AM stars? Rotation and rate of binaries among giant F stars". Astronomy and Astrophysics Supplement. 127 (2): 277–294. arXiv: astro-ph/9710226. Bibcode: 1998A&AS..127..277K. doi: 10.1051/aas:1998350. S2CID  7535170.
  15. ^ van Belle, Gerard T. (March 2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20 (1): 51, arXiv: 1204.2572, Bibcode: 2012A&ARv..20...51V, doi: 10.1007/s00159-012-0051-2, S2CID  119273474.
  16. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. Vizier catalog entry
Retrieved from " https://en.wikipedia.org/?title=16_Persei&oldid=1079512013"

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