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12 Pegasi

From Wikipedia, the free encyclopedia
K-type supergiant star in the constellation of Pegasus
12 Pegasi
Location of 12 Pegasi (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationPegasus
Right ascension21h 46m 04.364s[1]
Declination+22° 56′ 55.96″[1]
Apparent magnitude (V)+5.266[2]
Characteristics
Spectral typeK0IbHdel0.5[3]
U−Bcolor index+1.33[4]
B−Vcolor index+1.41[4]
Astrometry
Proper motion (μ)RA: 8.299[1]mas/yr
Dec.: −2.478[1]mas/yr
Parallax (π)2.3673±0.1279 mas[1]
Distance1,380 ± 70 ly
(420 ± 20 pc)
Absolute magnitude (MV)−4.03[4]
Details
Mass6.3[5] M
Radius81[6] R
Luminosity1,722–1,820[6] L
Surface gravity (log g)1.11[7] cgs
Temperature4,185[6] K
Metallicity [Fe/H]+0.03[7] dex
Rotational velocity (v sin i)19.5[8] km/s
Age19.8[5] Myr
Other designations
12 Peg,HR 8321,HD 207089,BD+22°4472,HIP 107472,SAO 89962
Database references
SIMBADdata

12 Pegasi is aK-type supergiant star in the constellation ofPegasus. It has aspectral type of K0Ib Hdel0.5,[9] which indicates that it is a less luminous K-type supergiant with strong H-δBalmer lines. The star has expanded to 81 times theradius of the Sun, and has aneffective temperature of 4,185 K.[6]

References

[edit]
  1. ^abcdeBrown, 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. ^Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^Keenan, Philip C.; McNeil, Raymond C. (October 1989). "The Perkins Catalog of Revised MK Types for the Cooler Stars".The Astrophysical Journal Supplement Series.71: 245.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.ISSN 0067-0049.
  4. ^abcMelnik, A. M.; Dambis, A. K. (2020). "VizieR Online Data Catalog: Kinematic data for high luminosity stars (Melnik+, 2020)".Vizier Online Data Catalog (Other).Bibcode:2020yCatp017036502M.
  5. ^abTetzlaff, N.; et al. (January 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.
  6. ^abcdMessineo, M.; Brown, A. G. A. (July 2019)."A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2".The Astronomical Journal.158 (1): 20.arXiv:1905.03744.Bibcode:2019AJ....158...20M.doi:10.3847/1538-3881/ab1cbd.ISSN 0004-6256.S2CID 148571616.
  7. ^abWu, Yue; et al. (2010). "Coudé-feed stellar spectral library – atmospheric parameters".Astronomy & Astrophysics.525: A71.arXiv:1009.1491.Bibcode:2011A&A...525A..71W.doi:10.1051/0004-6361/201015014.S2CID 53480665.
  8. ^De Medeiros, J. R.; Udry, S.; Burki, G.; Mayor, M. (2002)."A catalog of rotational and radial velocities for evolved stars. II. Ib supergiant stars"(PDF).Astronomy and Astrophysics.395:97–98.Bibcode:2002A&A...395...97D.doi:10.1051/0004-6361:20021214.
  9. ^Keenan, Philip C.; McNeil, Raymond C. (October 1989). "The Perkins catalog of revised MK types for the cooler stars".The Astrophysical Journal Supplement Series.71:245–266.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.ISSN 0067-0049.S2CID 123149047.
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