T Persei

T Persei is a red supergiant located in the constellation Perseus.

T Persei
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 2h 19m 21.87884s[1]
Declination +58° 57′ 40.3271″[1]
Apparent magnitude (V) 8.34-9.70[2]
Characteristics
Spectral type M2Iab[3]
U−B color index +2.62[4]
B−V color index +2.33[4]
Variable type SRc[2]
Astrometry
Radial velocity (Rv)−40.85[5] km/s
Proper motion (μ) RA: 0.31[1] mas/yr
Dec.: −2.42[1] mas/yr
Parallax (π)2.15 ± 1.24[1] mas
Distance2,345±55[6] pc
Absolute magnitude (MV)−6.90±0.07[6]
Details[6]
Mass9-12 M
Radius510±20 R
Luminosity45,700+4,400
−4,000
 L
Surface gravity (log g)0.06±0.05 cgs
Temperature3750±60 K
Metallicity [Fe/H]−0.35 dex
Other designations
T Per, HD 14142, HIP 10829, BD+58°439, WDS J02194+5858, 2MASS J02192186+5857403, AAVSO 0212+58
Database references
SIMBADdata

T Persei Media

References

  1. 1.0 1.1 1.2 1.3 1.4 Van Leeuwen, F.. Validation of the new Hipparcos reduction. Astronomy and Astrophysics 474 (2) (2007). p. 653–664. doi:10.1051/0004-6361:20078357.
  2. 2.0 2.1 Samus, N. N.. VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013). VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S 1 (2009).
  3. Kiss, L. L.. Variability in red supergiant stars: Pulsations, long secondary periods and convection noise. Monthly Notices of the Royal Astronomical Society 372 (4) (2006). p. 1721–1734. doi:10.1111/j.1365-2966.2006.10973.x.
  4. 4.0 4.1 Ducati, J. R.. VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system. CDS/ADC Collection of Electronic Catalogues 2237 (2002).
  5. Famaey, B.. Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters. Astronomy and Astrophysics 430 (2005). p. 165. doi:10.1051/0004-6361:20041272.
  6. 6.0 6.1 6.2 Baron, F.. Chara/mirc Observations of Two M Supergiants in Perseus Ob1: Temperature, Bayesian Modeling, and Compressed Sensing Imaging. The Astrophysical Journal 785 (1) (2014). p. 46. doi:10.1088/0004-637X/785/1/46.