From Wikipedia, the free encyclopedia
18 Aurigae
Observation data
Epoch J2000       Equinox J2000
Constellation Auriga
Right ascension 05h 19m 23.75342s [1]
Declination +33° 59′ 07.4035″ [1]
Apparent magnitude (V) 6.489 [2]
Characteristics
Spectral type A7 V [3]
U−B color index +0.09 [4]
B−V color index +0.256±0.007 [5]
Astrometry
Radial velocity (Rv)7.3±2 [6] km/s
Proper motion (μ) RA: +28.497 [1]  mas/ yr
Dec.: −12.714 [1]  mas/ yr
Parallax (π)14.0275 ± 0.0668  mas [1]
Distance233 ± 1  ly
(71.3 ± 0.3  pc)
Absolute magnitude (MV)2.31 [5]
Details
Mass1.69±0.03 [7]  M
Radius1.92+0.12
−0.03
[1]  R
Luminosity10.091±0.063 [1]  L
Surface gravity (log g)4.26±0.14  cgs
Temperature7,432+231
−67
[1]  K
Rotational velocity (v sin i)124 [7] km/s
Age950 [8]  Myr
Other designations
18 Aur, BD+33°1010, GC 6504, HD 34499, HIP 24832, HR 1734, SAO 57893, ADS 3893, WDS J05194+3359 [9]
Database references
SIMBAD data

18 Aurigae is a star located 233 [1]  light years away from the Sun in the northern constellation of Auriga. [9] The brightness of this object is near the limit of visibility to the naked eye under good viewing conditions, appearing as a dim, white-hued star with an apparent visual magnitude of 6.49. [2] The star is moving away from the Sun with a heliocentric radial velocity of 7 km/s. [6]

This is an ordinary A-type main-sequence star with a stellar classification of A7 V, [3] which indicates it is generating energy by hydrogen fusion at its core. The object is 950 [8] million years old with a high rate of spin, showing a projected rotational velocity of 124 km/s. [7] It has 1.7 [7] times the mass of the Sun and 1.9 [1] times the Sun's radius. The star is radiating 10 [1] times the luminosity of the Sun from its photosphere at an effective temperature of 7,432 K. [1]

18 Aurigae has a magnitude 12.50 companion star at an angular separation of 3.90 along a position angle of 167°, as of 2006. [10]

References

  1. ^ a b c d e f g h i j k l 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 Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H.
  3. ^ a b Cowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (1969). "A study of the bright stars. I. A catalogue of spectral classifications". The Astronomical Journal. 74: 375. Bibcode: 1969AJ.....74..375C. doi: 10.1086/110819.
  4. ^ Deutschman, W. A.; Davis, R. J.; Schild, R. E. (1976). "The galactic distribution of interstellar absorption as determined from the Celescope catalog of ultraviolet stellar observations and a new catalog of UBV, H-beta photoelectric observations". The Astrophysical Journal Supplement Series. 30: 97. Bibcode: 1976ApJS...30...97D. doi: 10.1086/190359.
  5. ^ 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.
  6. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode: 1953GCRV..C......0W.
  7. ^ a b c d Zorec, J.; et al. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. S2CID  55586789.
  8. ^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv: 1501.03154, Bibcode: 2015ApJ...804..146D, doi: 10.1088/0004-637X/804/2/146, S2CID  33401607.
  9. ^ a b "18 Aur". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-05-21.
  10. ^ Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920.

External links

From Wikipedia, the free encyclopedia
18 Aurigae
Observation data
Epoch J2000       Equinox J2000
Constellation Auriga
Right ascension 05h 19m 23.75342s [1]
Declination +33° 59′ 07.4035″ [1]
Apparent magnitude (V) 6.489 [2]
Characteristics
Spectral type A7 V [3]
U−B color index +0.09 [4]
B−V color index +0.256±0.007 [5]
Astrometry
Radial velocity (Rv)7.3±2 [6] km/s
Proper motion (μ) RA: +28.497 [1]  mas/ yr
Dec.: −12.714 [1]  mas/ yr
Parallax (π)14.0275 ± 0.0668  mas [1]
Distance233 ± 1  ly
(71.3 ± 0.3  pc)
Absolute magnitude (MV)2.31 [5]
Details
Mass1.69±0.03 [7]  M
Radius1.92+0.12
−0.03
[1]  R
Luminosity10.091±0.063 [1]  L
Surface gravity (log g)4.26±0.14  cgs
Temperature7,432+231
−67
[1]  K
Rotational velocity (v sin i)124 [7] km/s
Age950 [8]  Myr
Other designations
18 Aur, BD+33°1010, GC 6504, HD 34499, HIP 24832, HR 1734, SAO 57893, ADS 3893, WDS J05194+3359 [9]
Database references
SIMBAD data

18 Aurigae is a star located 233 [1]  light years away from the Sun in the northern constellation of Auriga. [9] The brightness of this object is near the limit of visibility to the naked eye under good viewing conditions, appearing as a dim, white-hued star with an apparent visual magnitude of 6.49. [2] The star is moving away from the Sun with a heliocentric radial velocity of 7 km/s. [6]

This is an ordinary A-type main-sequence star with a stellar classification of A7 V, [3] which indicates it is generating energy by hydrogen fusion at its core. The object is 950 [8] million years old with a high rate of spin, showing a projected rotational velocity of 124 km/s. [7] It has 1.7 [7] times the mass of the Sun and 1.9 [1] times the Sun's radius. The star is radiating 10 [1] times the luminosity of the Sun from its photosphere at an effective temperature of 7,432 K. [1]

18 Aurigae has a magnitude 12.50 companion star at an angular separation of 3.90 along a position angle of 167°, as of 2006. [10]

References

  1. ^ a b c d e f g h i j k l 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 Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H.
  3. ^ a b Cowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (1969). "A study of the bright stars. I. A catalogue of spectral classifications". The Astronomical Journal. 74: 375. Bibcode: 1969AJ.....74..375C. doi: 10.1086/110819.
  4. ^ Deutschman, W. A.; Davis, R. J.; Schild, R. E. (1976). "The galactic distribution of interstellar absorption as determined from the Celescope catalog of ultraviolet stellar observations and a new catalog of UBV, H-beta photoelectric observations". The Astrophysical Journal Supplement Series. 30: 97. Bibcode: 1976ApJS...30...97D. doi: 10.1086/190359.
  5. ^ 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.
  6. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode: 1953GCRV..C......0W.
  7. ^ a b c d Zorec, J.; et al. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. S2CID  55586789.
  8. ^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv: 1501.03154, Bibcode: 2015ApJ...804..146D, doi: 10.1088/0004-637X/804/2/146, S2CID  33401607.
  9. ^ a b "18 Aur". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-05-21.
  10. ^ Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920.

External links


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