From Wikipedia, the free encyclopedia
GX Velorum
Location of GX Velorum (circled)
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Vela
Right ascension 09h 11m 04.39802s [1]
Declination −44° 52′ 04.4411″ [1]
Apparent magnitude (V) +4.99 [2] (4.97 to 5.04) [3]
Characteristics
Spectral type B5 Ia [4]
U−B color index −0.57 [5]
B−V color index +0.22 [5]
Variable type α Cyg? [3]
Astrometry
Radial velocity (Rv)+28.2±0.8 [6] km/s
Proper motion (μ) RA: −5.608 [1]  mas/ yr
Dec.: +3.843 [1]  mas/ yr
Parallax (π)0.7696 ± 0.1585  mas [1]
Distanceapprox. 4,200  ly
(approx. 1,300  pc)
Absolute magnitude (MV)−7.20 [7]
Details [8]
Mass35  M
Radius61±7 [9]  R
Luminosity214,000 [9]  L
Surface gravity (log g)2.12±0.05 [9]  cgs
Temperature15,000±150 [9]  K
Rotational velocity (v sin i)39 km/s
Age8.3 [10]  Myr
Other designations
GX Vel, CD−44°5206, HD 79186, HIP 45085, HR 3654, SAO 220928 [11]
Database references
SIMBAD data

GX Velorum is a solitary [12] variable star [3] in the southern constellation of Vela. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude that fluctuates around 4.99. [2] Based upon parallax measurements, it is located approximately 4,200  light years distant from the Sun, and is drifting further away with a radial velocity of +28 km/s. [6] It may be a member of the Vela OB1 association of co-moving stars. [7]

A light curve for GX Velorum, plotted from Hipparcos data [13]

This object is a massive blue supergiant with a stellar classification of B5 Ia. [4] It is suspected to be an Alpha Cygni-type pulsating variable and ranges in brightness from 4.97 down to 5.04 magnitude. [3] It is losing mass at the rate of (0.40±0.02)×10−6 M yr−1, [9] or one solar mass every 2.5 million years. The star is 8.3 [10] million years old with 35 times the mass of the Sun. [8] It has expanded to around 61 [9] times the Sun's radius and is radiating 214,000 [9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 15,000 K. [9]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644.
  3. ^ a b c d Samus', N. N; et al. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. S2CID  125853869.
  4. ^ 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.
  5. ^ a b 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.
  6. ^ 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.
  7. ^ a b Reed, B. Cameron (2000). "Vela OB1: Probable New Members and Hertzsprung-Russell Diagram". The Astronomical Journal. 119 (4): 1855–1859. Bibcode: 2000AJ....119.1855R. doi: 10.1086/301313.
  8. ^ a b Fraser, M.; et al. (2010). "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants". Monthly Notices of the Royal Astronomical Society. 404 (3): 1306. arXiv: 1001.3337. Bibcode: 2010MNRAS.404.1306F. doi: 10.1111/j.1365-2966.2010.16392.x. S2CID  118674151.
  9. ^ a b c d e f g h Haucke, M.; et al. (June 2018), "Wind properties of variable B supergiants. Evidence of pulsations connected with mass-loss episodes", Astronomy & Astrophysics, 614: 28, arXiv: 1902.01341, Bibcode: 2018A&A...614A..91H, doi: 10.1051/0004-6361/201731678, S2CID  126150688, A91
  10. ^ a b 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.
  11. ^ "GX Vel". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-16.
  12. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID  14878976.
  13. ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
From Wikipedia, the free encyclopedia
GX Velorum
Location of GX Velorum (circled)
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Vela
Right ascension 09h 11m 04.39802s [1]
Declination −44° 52′ 04.4411″ [1]
Apparent magnitude (V) +4.99 [2] (4.97 to 5.04) [3]
Characteristics
Spectral type B5 Ia [4]
U−B color index −0.57 [5]
B−V color index +0.22 [5]
Variable type α Cyg? [3]
Astrometry
Radial velocity (Rv)+28.2±0.8 [6] km/s
Proper motion (μ) RA: −5.608 [1]  mas/ yr
Dec.: +3.843 [1]  mas/ yr
Parallax (π)0.7696 ± 0.1585  mas [1]
Distanceapprox. 4,200  ly
(approx. 1,300  pc)
Absolute magnitude (MV)−7.20 [7]
Details [8]
Mass35  M
Radius61±7 [9]  R
Luminosity214,000 [9]  L
Surface gravity (log g)2.12±0.05 [9]  cgs
Temperature15,000±150 [9]  K
Rotational velocity (v sin i)39 km/s
Age8.3 [10]  Myr
Other designations
GX Vel, CD−44°5206, HD 79186, HIP 45085, HR 3654, SAO 220928 [11]
Database references
SIMBAD data

GX Velorum is a solitary [12] variable star [3] in the southern constellation of Vela. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude that fluctuates around 4.99. [2] Based upon parallax measurements, it is located approximately 4,200  light years distant from the Sun, and is drifting further away with a radial velocity of +28 km/s. [6] It may be a member of the Vela OB1 association of co-moving stars. [7]

A light curve for GX Velorum, plotted from Hipparcos data [13]

This object is a massive blue supergiant with a stellar classification of B5 Ia. [4] It is suspected to be an Alpha Cygni-type pulsating variable and ranges in brightness from 4.97 down to 5.04 magnitude. [3] It is losing mass at the rate of (0.40±0.02)×10−6 M yr−1, [9] or one solar mass every 2.5 million years. The star is 8.3 [10] million years old with 35 times the mass of the Sun. [8] It has expanded to around 61 [9] times the Sun's radius and is radiating 214,000 [9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 15,000 K. [9]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644.
  3. ^ a b c d Samus', N. N; et al. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. S2CID  125853869.
  4. ^ 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.
  5. ^ a b 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.
  6. ^ 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.
  7. ^ a b Reed, B. Cameron (2000). "Vela OB1: Probable New Members and Hertzsprung-Russell Diagram". The Astronomical Journal. 119 (4): 1855–1859. Bibcode: 2000AJ....119.1855R. doi: 10.1086/301313.
  8. ^ a b Fraser, M.; et al. (2010). "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants". Monthly Notices of the Royal Astronomical Society. 404 (3): 1306. arXiv: 1001.3337. Bibcode: 2010MNRAS.404.1306F. doi: 10.1111/j.1365-2966.2010.16392.x. S2CID  118674151.
  9. ^ a b c d e f g h Haucke, M.; et al. (June 2018), "Wind properties of variable B supergiants. Evidence of pulsations connected with mass-loss episodes", Astronomy & Astrophysics, 614: 28, arXiv: 1902.01341, Bibcode: 2018A&A...614A..91H, doi: 10.1051/0004-6361/201731678, S2CID  126150688, A91
  10. ^ a b 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.
  11. ^ "GX Vel". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-16.
  12. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID  14878976.
  13. ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.

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