From Wikipedia, the free encyclopedia
6 Boötis

6 Boötis in optical light.
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Boötes
Right ascension 13h 49m 42.82223s [1]
Declination +21° 15′ 50.8580″ [1]
Apparent magnitude (V) 4.92 [2]
Characteristics
Spectral type K4 III [3] + M8 V [4]
B−V color index 1.432±0.013 [2]
Astrometry
Radial velocity (Rv)−3.71±0.48 [1] km/s
Proper motion (μ) RA: +33.773 [1]  mas/ yr
Dec.: +10.842 [1]  mas/ yr
Parallax (π)7.1527 ± 0.3659  mas [1]
Distance460 ± 20  ly
(140 ± 7  pc)
Absolute magnitude (MV)−0.49 [2]
Orbit [4]
Period (P)944±8 d
Eccentricity (e)0.41±0.09
Periastron epoch (T)2,444,739.5±31.0  JD
Argument of periastron (ω)
(secondary)
359±15°
Semi-amplitude (K1)
(primary)
1.19±0.15 km/s
Details
Radius38 [5]  R
Luminosity430.124 [1]  L
Surface gravity (log g)1.910 [6]  cgs
Temperature4,050 [6]  K
Metallicity [Fe/H]−0.24 [6]  dex
Rotational velocity (v sin i)2.0 [7] km/s
Other designations
e Boötis, 53 Cam, BD+21°2578, FK5 3098, GC 18683, HD 120539, HIP 67480, HR 5201, SAO 83015 [8]
Database references
SIMBAD data

6 Boötis is a binary star [4] system in the northern constellation of Boötes, [8] located around 460  light years away from the Sun. [1] It has the Bayer designation e Boötis; 6 Boötis is the Flamsteed designation. [8] The system is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.92. [2] It is moving closer to the Earth with a heliocentric radial velocity of −3 km/s. [2]

This is a single-lined spectroscopic binary system with an orbital period of 2.58 years and an eccentricity of 0.4. [4] The visible component is an evolved giant star with a stellar classification of K4 III. [3] Its measured angular diameter is 2.53±0.12  mas. [9] At the estimated distance of the star, this yields a physical size of about 38 times the radius of the Sun. [5] The star is radiating 430 [1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,050 K. [6] Its companion is probably a low mass red dwarf of around class M8 V. [4]

References

  1. ^ a b c d e f g h i 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 e 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 Yoss, K. M.; Griffin, R. F. (September 1997), "Radial Velocities and DDO, BV Photometry of Henry Draper G5-M Stars Near the North Galactic Pole", Journal of Astrophysics and Astronomy, 18 (2–3): 161, Bibcode: 1997JApA...18..161Y, doi: 10.1007/BF02714877, S2CID  123221180.
  4. ^ a b c d e Griffin, R. F. (June 1985), "Spectroscopic binaries near the North Galactic Pole. Paper 12 : 6 Bootis.", Journal of Astrophysics and Astronomy, 6: 77–83, Bibcode: 1985JApA....6...77G, doi: 10.1007/BF02715079, S2CID  124682374.
  5. ^ 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:
  6. ^ a b c d McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode: 1990ApJS...74.1075M, doi: 10.1086/191527
  7. ^ De Medeiros, J. R.; et al. (October 2002), "The Rotation of Binary Systems with Evolved Components", The Astrophysical Journal, 578 (2): 943–950, arXiv: astro-ph/0207288, Bibcode: 2002ApJ...578..943D, doi: 10.1086/342613, S2CID  16196039.
  8. ^ a b c "6 Boo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-23.
  9. ^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039.
From Wikipedia, the free encyclopedia
6 Boötis

6 Boötis in optical light.
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Boötes
Right ascension 13h 49m 42.82223s [1]
Declination +21° 15′ 50.8580″ [1]
Apparent magnitude (V) 4.92 [2]
Characteristics
Spectral type K4 III [3] + M8 V [4]
B−V color index 1.432±0.013 [2]
Astrometry
Radial velocity (Rv)−3.71±0.48 [1] km/s
Proper motion (μ) RA: +33.773 [1]  mas/ yr
Dec.: +10.842 [1]  mas/ yr
Parallax (π)7.1527 ± 0.3659  mas [1]
Distance460 ± 20  ly
(140 ± 7  pc)
Absolute magnitude (MV)−0.49 [2]
Orbit [4]
Period (P)944±8 d
Eccentricity (e)0.41±0.09
Periastron epoch (T)2,444,739.5±31.0  JD
Argument of periastron (ω)
(secondary)
359±15°
Semi-amplitude (K1)
(primary)
1.19±0.15 km/s
Details
Radius38 [5]  R
Luminosity430.124 [1]  L
Surface gravity (log g)1.910 [6]  cgs
Temperature4,050 [6]  K
Metallicity [Fe/H]−0.24 [6]  dex
Rotational velocity (v sin i)2.0 [7] km/s
Other designations
e Boötis, 53 Cam, BD+21°2578, FK5 3098, GC 18683, HD 120539, HIP 67480, HR 5201, SAO 83015 [8]
Database references
SIMBAD data

6 Boötis is a binary star [4] system in the northern constellation of Boötes, [8] located around 460  light years away from the Sun. [1] It has the Bayer designation e Boötis; 6 Boötis is the Flamsteed designation. [8] The system is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.92. [2] It is moving closer to the Earth with a heliocentric radial velocity of −3 km/s. [2]

This is a single-lined spectroscopic binary system with an orbital period of 2.58 years and an eccentricity of 0.4. [4] The visible component is an evolved giant star with a stellar classification of K4 III. [3] Its measured angular diameter is 2.53±0.12  mas. [9] At the estimated distance of the star, this yields a physical size of about 38 times the radius of the Sun. [5] The star is radiating 430 [1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,050 K. [6] Its companion is probably a low mass red dwarf of around class M8 V. [4]

References

  1. ^ a b c d e f g h i 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 e 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 Yoss, K. M.; Griffin, R. F. (September 1997), "Radial Velocities and DDO, BV Photometry of Henry Draper G5-M Stars Near the North Galactic Pole", Journal of Astrophysics and Astronomy, 18 (2–3): 161, Bibcode: 1997JApA...18..161Y, doi: 10.1007/BF02714877, S2CID  123221180.
  4. ^ a b c d e Griffin, R. F. (June 1985), "Spectroscopic binaries near the North Galactic Pole. Paper 12 : 6 Bootis.", Journal of Astrophysics and Astronomy, 6: 77–83, Bibcode: 1985JApA....6...77G, doi: 10.1007/BF02715079, S2CID  124682374.
  5. ^ 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:
  6. ^ a b c d McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode: 1990ApJS...74.1075M, doi: 10.1086/191527
  7. ^ De Medeiros, J. R.; et al. (October 2002), "The Rotation of Binary Systems with Evolved Components", The Astrophysical Journal, 578 (2): 943–950, arXiv: astro-ph/0207288, Bibcode: 2002ApJ...578..943D, doi: 10.1086/342613, S2CID  16196039.
  8. ^ a b c "6 Boo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-23.
  9. ^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039.

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