PV Telescopii

HD 168476
Observation data
Epoch J2000      Equinox J2000
Constellation Telescopium
Right ascension 18h 23m 14.6635s
Declination -56° 37 44.15
Apparent magnitude (V) 9.25
Characteristics
Spectral type B5p
B−V color index -0.01
Variable type PV Tel
Astrometry
Radial velocity (Rv)-169 km/s
Proper motion (μ) RA: 0.38 mas/yr
Dec.: -9.29 mas/yr
Parallax (π)0.43 ± 1.12 mas
Distanceapprox. 10,000 ly
(approx. 2,000 pc)
Absolute magnitude (MV)-2.25
Details
Mass0.9[1] M
Radius19[2] R
Luminosity~6,500 L
Surface gravity (log g)1.5[3] cgs
Temperature14,000[3] K
Metallicity-0.15[3]
Other designations
PV Telescopii, PV Tel, HD 168476, HIP 90099.
Database references
SIMBADdata

PV Telescopii (also known as HD 168476) is a class B-type (blue) extreme helium star in the constelation Telescopium. It is also the prototype of variable stars called PV Telescopii variables. These are probably post-AGB stars with weak Hydrogen lines and enhanced Helium and Carbon lines. Their variable periods are from a few hours to a few years and as of 2008, there are 12 confirmed PV Telescopii variables. Some researchers have modelled white dwarf mergers as a way to produce these unlikely stars.[4]

References

  1. Jeffery, C. S.; Starling, R. L. C.; Hill, P. W.; Pollacco, D. (2001). "Cyclic and secular variation in the temperatures and radii of extreme helium stars". Monthly Notices of the Royal Astronomical Society 321: 111. doi:10.1046/j.1365-8711.2001.03992.x.
  2. Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition -Comments and statistics". Astronomy and Astrophysics 367 (2): 521. doi:10.1051/0004-6361:20000451.
  3. 3.0 3.1 3.2 Soubiran, C.; Le Campion, J. -F.; Cayrel De Strobel, G.; Caillo, A. (2010). "The PASTEL catalogue of stellar parameters". Astronomy and Astrophysics 515: A111. Bibcode:2010A&A...515A.111S. doi:10.1051/0004-6361/201014247.
  4. Gourgouliatos, K. N.; Jeffery, C. S. (2006). "On the angular momentum evolution of merged white dwarfs". Monthly Notices of the Royal Astronomical Society 371 (3): 1381. doi:10.1111/j.1365-2966.2006.10780.x.

See also