Langbahn Team – Weltmeisterschaft

HD 64740

HD 64740
Location of HD 64740 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 53m 03.63538s[1]
Declination −49° 36′ 46.9530″[1]
Apparent magnitude (V) 4.63[2]
Characteristics
Spectral type B2V[3]
U−B color index −0.92[2]
B−V color index −0.23[2]
Variable type Constant[4]
Astrometry
Radial velocity (Rv)+8.00±4.2[5] km/s
Proper motion (μ) RA: −7.77[1] mas/yr
Dec.: +15.16[1] mas/yr
Parallax (π)4.30 ± 0.15 mas[1]
Distance760 ± 30 ly
(233 ± 8 pc)
Absolute magnitude (MV)−2.2±0.1[6]
Details
Mass9.6 M☉[7]
10.1±0.5[8] M☉
Radius4.5±0.7[8] R☉
Luminosity5,908[9] L☉
Surface gravity (log g)4.01±0.09[6] cgs
Temperature23,700[9] K
Metallicity [Fe/H]+0.01[10] dex
Rotation1.33026 d[11]
Rotational velocity (v sin i)160[12] km/s
Age12.6+7.4
−2.7[8] Myr
Other designations
CD−49°3137, CPD−49°1398, GC 10686, HD 64740, HIP 38500, HR 3089, SAO 219106, GSC 08143-03240
Database references
SIMBADdata

HD 64740 is a single[13] star in the southern constellation Puppis, positioned near the line of sight to the Gum Nebula.[4] It has a blue-white hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.63.[2] Parallax measurements give a distance estimate of approximately 760 light-years from the Sun,[1] and it is drifting further away with a radial velocity of +8 km/s.[5]

This is a massive B-type main-sequence star with a stellar classification of B2V.[3] It is a magnetic chemically peculiar star of the helium strong variety[6] with weak hydrogen alpha emission.[8] The polar magnetic field strength is 3,700 G.[4] The star is about halfway through its main sequence lifetime with an estimated age of ~13 million years.[8] It is spinning rapidly with an equatorial velocity of about 140±10 km/s, based on a polar inclination angle of 36°±15°,[4] giving it a rotation period of ~1.33 days.[11] The star is radiating over 5,900 times the luminosity of the Sun from its photosphere at an effective temperature of 23,700 K.[9]

Significant X-ray emission has been detected originating from this star, which may be connected to the magnetically-confined stellar wind.[14] The star does not display pulsation behavior, but it does show a magnetically-modulated variation from the wind.[15] Variation of ultraviolet lines of silicon has been detected, which may be due to surface abundance variations.[4] Two patches of helium overabundance are observed near the magnetic poles, which are inclined by about 20° to the star's pole of rotation.[11]

References

  1. ^ a b c d e f Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  2. ^ a b c d 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.
  3. ^ a b Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  4. ^ a b c d e Krtička, J.; et al. (August 2013). "Ultraviolet and visual flux and line variations of one of the least variable Bp stars HD 64740". Astronomy & Astrophysics. 556: 11. arXiv:1306.2458. Bibcode:2013A&A...556A..18K. doi:10.1051/0004-6361/201221018. S2CID 73647737. A18.
  5. ^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  6. ^ a b c Shultz, M. E.; et al. (May 2019). "The magnetic early B-type Stars II: stellar atmospheric parameters in the era of Gaia". Monthly Notices of the Royal Astronomical Society. 485 (2): 1508–1527. arXiv:1902.02713. Bibcode:2019MNRAS.485.1508S. doi:10.1093/mnras/stz416.
  7. ^ Tetzlaff, N.; et al. (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. Vizier catalog entry
  8. ^ a b c d e Shultz, M. E.; et al. (November 2019). "The magnetic early B-type stars - III. A main-sequence magnetic, rotational, and magnetospheric biography". Monthly Notices of the Royal Astronomical Society. 490 (1): 274–295. arXiv:1909.02530. Bibcode:2019MNRAS.490..274S. doi:10.1093/mnras/stz2551.
  9. ^ a b c Hohle, M. M.; et al. (2010). "Masses and luminosities of O- and B-type stars and red supergiants". Astronomische Nachrichten. 331 (4): 349. arXiv:1003.2335. Bibcode:2010AN....331..349H. doi:10.1002/asna.200911355. S2CID 111387483. Vizier catalog entry
  10. ^ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. S2CID 118345778. Vizier catalog entry
  11. ^ a b c Alecian, E.; et al. (December 2012). Boissier, S.; et al. (eds.). The Magnetism in Massive Stars (MiMeS) project: First HARPSpol discoveries. Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. pp. 401–404. arXiv:1211.1075. Bibcode:2012sf2a.conf..401A.
  12. ^ Hoffleit, D.; Warren, W. H. (1995). "Bright Star Catalogue". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050 (5th Revised ed.). Bibcode:1995yCat.5050....0H.
  13. ^ Chini, R.; et al. (2012). "A spectroscopic survey on the multiplicity of high-mass stars". Monthly Notices of the Royal Astronomical Society. 424 (3): 1925. arXiv:1205.5238. Bibcode:2012MNRAS.424.1925C. doi:10.1111/j.1365-2966.2012.21317.x. S2CID 119120749.
  14. ^ Nazé, Yaël; et al. (November 2014). "X-Ray Emission from Magnetic Massive Stars". The Astrophysical Journal Supplement. 215 (1): 20. arXiv:1409.1690. Bibcode:2014ApJS..215...10N. doi:10.1088/0067-0049/215/1/10. S2CID 54074229. 10.
  15. ^ Telting, J. H.; et al. (2006). "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars". Astronomy and Astrophysics. 452 (3): 945. Bibcode:2006A&A...452..945T. doi:10.1051/0004-6361:20054730. hdl:2066/36162.
Quelle: http://en.wikipedia.org/wiki/HD_64740