From Wikipedia, the free encyclopedia
δ Fornacis
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Fornax
Right ascension 03h 42m 14.90238s [1]
Declination −31° 56′ 18.0961″ [1]
Apparent magnitude (V) 5.00 [2]
Characteristics
Spectral type B5 III [3]
U−B color index −0.60 [2]
B−V color index −0.16 [2]
Astrometry
Radial velocity (Rv)+26.00 [4] km/s
Proper motion (μ) RA: +4.942 [1]  mas/ yr
Dec.: +13.326 [1]  mas/ yr
Parallax (π)4.1125 ± 0.2114  mas [1]
Distance790 ± 40  ly
(240 ± 10  pc)
Absolute magnitude (MV)−2.07 [5]
Details
Mass5.9±0.2 [6]  M
Radius6.0 [7]  R
Luminosity1,291 [8]  L
Temperature16,230±930 [9]  K
Rotational velocity (v sin i)185 [10] km/s
Age63.1±16.1 [6]  Myr
Other designations
δ For, CD−32° 1430, FK5 133, HD 23227, HIP 17304, HR 1134, SAO 194467 [11]
Database references
SIMBAD data

Delta Fornacis, Latinized from δ Fornacis, is a solitary, [12] blue-white hued star near the middle of the southern constellation of Fornax. With an apparent visual magnitude of 5.00, [2] it is faintly visible to the naked eye at night. The star has an annual parallax shift of 4.1  mas, [1] indicating it lies at a distance of approximately 790  light years from the Sun. It is drifting further away with a radial velocity of +26 km/s. [4]

The stellar classification of Delta Fornacis is B5 III, [3] matching an evolved B-type giant star. It has an angular diameter of 0.215±0.015 mas, [9] which, at the estimated distance of the star, yields a physical size of around 6 times the radius of the Sun. [7] Around 63 million years old, [6] the star is spinning rapidly with a projected rotational velocity of 185 km/s. [10] It has an estimated 5.9 [6] times the Sun's mass and radiates 1,291 [8] times the solar luminosity from its outer atmosphere at an effective temperature of 16,230 K. [9]

References

  1. ^ a b c d e f 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 c d Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1999), "UBVRIJKL photometry of the bright stars", Commission Lunar and Planetary Laboratory, 4: 99, Bibcode: 1966CoLPL...4...99J.
  3. ^ a b Houk, N. (1982), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1982mcts.book.....H.
  4. ^ a b Kharchenko, N. V.; et al. (2007), "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations", Astronomische Nachrichten, 328 (9): 889, arXiv: 0705.0878, Bibcode: 2007AN....328..889K, doi: 10.1002/asna.200710776, S2CID  119323941.
  5. ^ 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.
  6. ^ a b c d Tetzlaff, N.; et al. (January 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.
  7. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  8. ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID  118665352.
  9. ^ a b c Zorec, J.; et al. (2009), "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff", Astronomy and Astrophysics, 501 (1): 297–320, arXiv: 0903.5134, Bibcode: 2009A&A...501..297Z, doi: 10.1051/0004-6361/200811147, S2CID  14969137.
  10. ^ a b Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590.
  11. ^ "del For". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-17.
  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.
From Wikipedia, the free encyclopedia
δ Fornacis
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Fornax
Right ascension 03h 42m 14.90238s [1]
Declination −31° 56′ 18.0961″ [1]
Apparent magnitude (V) 5.00 [2]
Characteristics
Spectral type B5 III [3]
U−B color index −0.60 [2]
B−V color index −0.16 [2]
Astrometry
Radial velocity (Rv)+26.00 [4] km/s
Proper motion (μ) RA: +4.942 [1]  mas/ yr
Dec.: +13.326 [1]  mas/ yr
Parallax (π)4.1125 ± 0.2114  mas [1]
Distance790 ± 40  ly
(240 ± 10  pc)
Absolute magnitude (MV)−2.07 [5]
Details
Mass5.9±0.2 [6]  M
Radius6.0 [7]  R
Luminosity1,291 [8]  L
Temperature16,230±930 [9]  K
Rotational velocity (v sin i)185 [10] km/s
Age63.1±16.1 [6]  Myr
Other designations
δ For, CD−32° 1430, FK5 133, HD 23227, HIP 17304, HR 1134, SAO 194467 [11]
Database references
SIMBAD data

Delta Fornacis, Latinized from δ Fornacis, is a solitary, [12] blue-white hued star near the middle of the southern constellation of Fornax. With an apparent visual magnitude of 5.00, [2] it is faintly visible to the naked eye at night. The star has an annual parallax shift of 4.1  mas, [1] indicating it lies at a distance of approximately 790  light years from the Sun. It is drifting further away with a radial velocity of +26 km/s. [4]

The stellar classification of Delta Fornacis is B5 III, [3] matching an evolved B-type giant star. It has an angular diameter of 0.215±0.015 mas, [9] which, at the estimated distance of the star, yields a physical size of around 6 times the radius of the Sun. [7] Around 63 million years old, [6] the star is spinning rapidly with a projected rotational velocity of 185 km/s. [10] It has an estimated 5.9 [6] times the Sun's mass and radiates 1,291 [8] times the solar luminosity from its outer atmosphere at an effective temperature of 16,230 K. [9]

References

  1. ^ a b c d e f 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 c d Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1999), "UBVRIJKL photometry of the bright stars", Commission Lunar and Planetary Laboratory, 4: 99, Bibcode: 1966CoLPL...4...99J.
  3. ^ a b Houk, N. (1982), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1982mcts.book.....H.
  4. ^ a b Kharchenko, N. V.; et al. (2007), "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations", Astronomische Nachrichten, 328 (9): 889, arXiv: 0705.0878, Bibcode: 2007AN....328..889K, doi: 10.1002/asna.200710776, S2CID  119323941.
  5. ^ 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.
  6. ^ a b c d Tetzlaff, N.; et al. (January 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.
  7. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  8. ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID  118665352.
  9. ^ a b c Zorec, J.; et al. (2009), "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff", Astronomy and Astrophysics, 501 (1): 297–320, arXiv: 0903.5134, Bibcode: 2009A&A...501..297Z, doi: 10.1051/0004-6361/200811147, S2CID  14969137.
  10. ^ a b Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590.
  11. ^ "del For". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-17.
  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.

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