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29 Camelopardalis
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Camelopardalis
Right ascension 05h 50m 33.8729s [1]
Declination +56° 55′ 08.1822″ [1]
Apparent magnitude (V) 6.590±0.009 [2]
Characteristics
29 Cam A
Spectral type A4 IV-V
U−B color index +0.13 [2]
B−V color index +0.09 [2]
29 Cam B
Spectral type A3 V
Astrometry
29 Cam A
Radial velocity (Rv)3.9±2 [3] km/s
Proper motion (μ) RA: –19.460 [1]  mas/ yr
Dec.: –4.249 [1]  mas/ yr
Parallax (π)6.7370 ± 0.0607  mas [1]
Distance484 ± 4  ly
(148 ± 1  pc)
Absolute magnitude (MV)+0.71 [4]
29 Cam B
Proper motion (μ) RA: +2.585 [5]  mas/ yr
Dec.: –0.570 [5]  mas/ yr
Parallax (π)1.6375 ± 0.0483  mas [5]
Distance1,990 ± 60  ly
(610 ± 20  pc)
Details
29 Cam A
Mass2.47 ± 0.08 [6]  M☉
Radius3.49+0.14
−0.12 [7]  R☉
Luminosity58.9+8.9
−7.6 [6]  L☉
Surface gravity (log g)3.77 [8]  cgs
Temperature8,337 ± 96 [6]  K
Rotational velocity (v sin i)123 [9] km/s
Age380 ± 14 [6]  Myr
29 Cam B
Mass2.12 [10]  M☉
Radius2.06 [11]  R☉
Luminosity15.043 [11]  L☉
Temperature7911 [11]  K
Rotational velocity (v sin i)110±8 [12] km/s
Other designations
BD+56° 1065, HD 38618, HIP 27592, HR 1992, SAO 25403, WDS J05506+5655A
Database references
SIMBAD data

29 Camelopardalis (29 Cam) is a double star in the circumpolar constellation Camelopardalis. With an apparent magnitude of 6.59, [2] it's right below the max visibility to the naked eye, and can only be viewed under phenomenal conditions. The star is located 484 light years [1] away based on parallax, but is drifting further away with a radial velocity of 3.9 km/s. [3]

29 Cam A

29 Cam A has a classification of A4IV-V, which suggests that this star is beginning to evolve off the main sequence. Zorec et al. models it as a star that has completed 90.6% of the main sequence, which correlates to an age of 380 million years. [6] At present, 29 Cam has 2.47 the mass of the Sun, [6] and 3.49 times its radius. [7] It radiates at 58.9 times the luminosity of the Sun from an effective temperature of 8,337 K, [6] which gives it a white hue of an A-type star. 29 Cam spins rapidly at a projected rotational velocity of 123 km/s despite its evolved state.

29 Cam B

29 Cam has a companion designated BD+56 1065B, which is a 10 magnitude star. According to the proper motion, this star is unrelated to the primary, and is 4 times farther than the primary. [13] The companion is relatively cooler and less luminous than the primary.

References

  1. ^ a b c d e f Brown, 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 at VizieR.
  2. ^ a b c d Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series. 89: 415–419. Bibcode: 1991A&AS...89..415O. ISSN  0365-0138.
  3. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication. Bibcode: 1953GCRV..C......0W.
  4. ^ 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. ISSN  1063-7737. S2CID  119257644.
  5. ^ a b c Brown, 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 at VizieR.
  6. ^ a b c d e f g Zorec, J.; Royer, F. (1 January 2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. ISSN  0004-6361. S2CID  55586789.
  7. ^ a b Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara (October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. hdl: 1721.1/124721. ISSN  0004-6256. S2CID  166227927.
  8. ^ Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevic, G.; Monari, G.; Cantat-Gaudin, T. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ Royer, 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 and Astrophysics. 393: 897–911. arXiv: astro-ph/0205255. Bibcode: 2002A&A...393..897R. doi: 10.1051/0004-6361:20020943. ISSN  0004-6361.
  10. ^ Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara (2019-10-01). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. hdl: 1721.1/124721. ISSN  0004-6256. S2CID  166227927.
  11. ^ a b c Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; Babusiaux, C.; Bailer-Jones, C. A. L.; Biermann, M.; Evans, D. W.; Eyer, L.; Jansen, F. (2018-08-01). "Gaia Data Release 2. Summary of the contents and survey properties". Astronomy and Astrophysics. 616: A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. ISSN  0004-6361.
  12. ^ Glebocki, R.; Gnacinski, P. (2005-03-01). "Systematic errors in the determination of stellar rotational velocities". 13th Cambridge Workshop on Cool Stars. 560: 571. Bibcode: 2005ESASP.560..571G.
  13. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001-12-01). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. ISSN  0004-6256. S2CID  119533755.


Stub icon

This subgiant-star-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from " https://en.wikipedia.org/?title=29_Camelopardalis&oldid=1187254850"
From Wikipedia, the free encyclopedia
29 Camelopardalis
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Camelopardalis
Right ascension 05h 50m 33.8729s [1]
Declination +56° 55′ 08.1822″ [1]
Apparent magnitude (V) 6.590±0.009 [2]
Characteristics
29 Cam A
Spectral type A4 IV-V
U−B color index +0.13 [2]
B−V color index +0.09 [2]
29 Cam B
Spectral type A3 V
Astrometry
29 Cam A
Radial velocity (Rv)3.9±2 [3] km/s
Proper motion (μ) RA: –19.460 [1]  mas/ yr
Dec.: –4.249 [1]  mas/ yr
Parallax (π)6.7370 ± 0.0607  mas [1]
Distance484 ± 4  ly
(148 ± 1  pc)
Absolute magnitude (MV)+0.71 [4]
29 Cam B
Proper motion (μ) RA: +2.585 [5]  mas/ yr
Dec.: –0.570 [5]  mas/ yr
Parallax (π)1.6375 ± 0.0483  mas [5]
Distance1,990 ± 60  ly
(610 ± 20  pc)
Details
29 Cam A
Mass2.47 ± 0.08 [6]  M☉
Radius3.49+0.14
−0.12 [7]  R☉
Luminosity58.9+8.9
−7.6 [6]  L☉
Surface gravity (log g)3.77 [8]  cgs
Temperature8,337 ± 96 [6]  K
Rotational velocity (v sin i)123 [9] km/s
Age380 ± 14 [6]  Myr
29 Cam B
Mass2.12 [10]  M☉
Radius2.06 [11]  R☉
Luminosity15.043 [11]  L☉
Temperature7911 [11]  K
Rotational velocity (v sin i)110±8 [12] km/s
Other designations
BD+56° 1065, HD 38618, HIP 27592, HR 1992, SAO 25403, WDS J05506+5655A
Database references
SIMBAD data

29 Camelopardalis (29 Cam) is a double star in the circumpolar constellation Camelopardalis. With an apparent magnitude of 6.59, [2] it's right below the max visibility to the naked eye, and can only be viewed under phenomenal conditions. The star is located 484 light years [1] away based on parallax, but is drifting further away with a radial velocity of 3.9 km/s. [3]

29 Cam A

29 Cam A has a classification of A4IV-V, which suggests that this star is beginning to evolve off the main sequence. Zorec et al. models it as a star that has completed 90.6% of the main sequence, which correlates to an age of 380 million years. [6] At present, 29 Cam has 2.47 the mass of the Sun, [6] and 3.49 times its radius. [7] It radiates at 58.9 times the luminosity of the Sun from an effective temperature of 8,337 K, [6] which gives it a white hue of an A-type star. 29 Cam spins rapidly at a projected rotational velocity of 123 km/s despite its evolved state.

29 Cam B

29 Cam has a companion designated BD+56 1065B, which is a 10 magnitude star. According to the proper motion, this star is unrelated to the primary, and is 4 times farther than the primary. [13] The companion is relatively cooler and less luminous than the primary.

References

  1. ^ a b c d e f Brown, 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 at VizieR.
  2. ^ a b c d Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series. 89: 415–419. Bibcode: 1991A&AS...89..415O. ISSN  0365-0138.
  3. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication. Bibcode: 1953GCRV..C......0W.
  4. ^ 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. ISSN  1063-7737. S2CID  119257644.
  5. ^ a b c Brown, 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 at VizieR.
  6. ^ a b c d e f g Zorec, J.; Royer, F. (1 January 2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. ISSN  0004-6361. S2CID  55586789.
  7. ^ a b Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara (October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. hdl: 1721.1/124721. ISSN  0004-6256. S2CID  166227927.
  8. ^ Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevic, G.; Monari, G.; Cantat-Gaudin, T. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ Royer, 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 and Astrophysics. 393: 897–911. arXiv: astro-ph/0205255. Bibcode: 2002A&A...393..897R. doi: 10.1051/0004-6361:20020943. ISSN  0004-6361.
  10. ^ Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara (2019-10-01). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. hdl: 1721.1/124721. ISSN  0004-6256. S2CID  166227927.
  11. ^ a b c Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; Babusiaux, C.; Bailer-Jones, C. A. L.; Biermann, M.; Evans, D. W.; Eyer, L.; Jansen, F. (2018-08-01). "Gaia Data Release 2. Summary of the contents and survey properties". Astronomy and Astrophysics. 616: A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. ISSN  0004-6361.
  12. ^ Glebocki, R.; Gnacinski, P. (2005-03-01). "Systematic errors in the determination of stellar rotational velocities". 13th Cambridge Workshop on Cool Stars. 560: 571. Bibcode: 2005ESASP.560..571G.
  13. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001-12-01). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. ISSN  0004-6256. S2CID  119533755.


Stub icon

This subgiant-star-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from " https://en.wikipedia.org/?title=29_Camelopardalis&oldid=1187254850"

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