PV Telescopii
PV Telescopii (also known as HD 168476) is a class B-type (blue) supergiant extreme helium star in the constellation Telescopium. It is also the prototype of variable stars called PV Telescopii variables.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Telescopium |
Right ascension | 18h 23m 14.66390s[1] |
Declination | −56° 37′ 44.1512″[1] |
Apparent magnitude (V) | 9.30[2] (9.24 - 9.40[3]) |
Characteristics | |
Spectral type | B5p[4] |
U−B color index | −0.60[2] |
B−V color index | −0.10[2] |
Variable type | PV Tel[3] |
Astrometry | |
Radial velocity (Rv) | -169[5] km/s |
Proper motion (μ) | RA: 0.38[1] mas/yr Dec.: -9.29[1] mas/yr |
Parallax (π) | 0.43 ± 1.12[1] mas |
Distance | 8,000[6] pc |
Absolute magnitude (MV) | −4.4[7] |
Details | |
Mass | 0.94[6] M☉ |
Radius | 33.9[6] R☉ |
Luminosity | 25,000[6] L☉ |
Surface gravity (log g) | 1.35[6] cgs |
Temperature | 12,425[6] K |
Metallicity | -0.15[8] |
Other designations | |
Database references | |
SIMBAD | data |
Properties
PV Telescopii shows radial velocity changes thought to be due to radial pulsations caused by a strange mode instability[6] It appears as a star of magnitude 9.3. Despite a mass thought to be less than the sun, it is actually around 25,000 more luminous. The spectrum shows a strong hydrogen deficiency and strongly enhanced helium and carbon lines.[9]
PV Telescopii variable
PV Telescopii variables are helium supergiants which vary somewhat irregularly over about 0.1 magnitude on a time-scale of hours to days. PV Telescopii is an example with variations over a few days, 8–10 days being typically quoted. It may be a late thermal pulse post-AGB star or the result of a white dwarf merger.[6][10]
References
- Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
- Samus, N. N.; Durlevich, O. V.; et al. (2009). "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. Bibcode:2009yCat....102025S.
- Walker, H. J.; Hill, P. W. (1985). "Radial velocities for the hydrogen-deficient star HD 168476, several helium-strong and helium-weak stars". Astronomy and Astrophysics Supplement Series. 61: 303. Bibcode:1985A&AS...61..303W.
- Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
- 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. Bibcode:2001MNRAS.321..111J. CiteSeerX 10.1.1.29.1648. doi:10.1046/j.1365-8711.2001.03992.x.
- Heber, U.; Schoenberner, D. (1981). "Colours and effective temperatures of extreme helium stars". Astronomy and Astrophysics. 102: 73. Bibcode:1981A&A...102...73H.
- Soubiran, C.; Le Campion, J. -F.; Cayrel De Strobel, G.; Caillo, A. (2010). "The PASTEL catalogue of stellar parameters". Astronomy and Astrophysics. 515: A111. arXiv:1004.1069. Bibcode:2010A&A...515A.111S. doi:10.1051/0004-6361/201014247.
- Pandey, Gajendra; Lambert, David L. (2011). "Neon and CNO Abundances for Extreme Helium Stars—A Non-LTE Analysis". The Astrophysical Journal. 727 (2): 122. arXiv:1011.5035. Bibcode:2011ApJ...727..122P. doi:10.1088/0004-637X/727/2/122.
- 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. arXiv:astro-ph/0607379. Bibcode:2006MNRAS.371.1381G. doi:10.1111/j.1365-2966.2006.10780.x.