From Wikipedia, the free encyclopedia
11 Canis Majoris
Observation data
Epoch J2000       Equinox J2000
Constellation Canis Major
Right ascension 06h 46m 51.09272s [1]
Declination −14° 25′ 33.5042″ [1]
Apparent magnitude (V) 5.28 [2]
Characteristics
Spectral type B8/9III [3]
B−V color index −0.024±0.004 [2]
Astrometry
Radial velocity (Rv)+15.0±4.2 [4] km/s
Proper motion (μ) RA: −2.853±0.344 [1]  mas/ yr
Dec.: +8.514±0.363 [1]  mas/ yr
Parallax (π)3.2263 ± 0.1847  mas [1]
Distance1,010 ± 60  ly
(310 ± 20  pc)
Absolute magnitude (MV)−1.63 [2]
Details
Luminosity485.12 [2]  L
Temperature11,540±181 [5]  K
Rotational velocity (v sin i)130 [5] km/s
Other designations
11 CMa, BD−14°1584, GC 8879, HD 49229, HIP 32492, HR 2504, SAO 151919 [6]
Database references
SIMBAD data

11 Canis Majoris is a single [7] star in the southern constellation of Canis Major, the eleventh entry in John Flamsteed's catalogue of stars in that constellation. It has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of 5.28. [2] The distance to this star is approximately 1,010  light years from the Sun based on parallax, [1] and it is drifting further away with a radial velocity of around +15 km/s. [4] It has an absolute magnitude of −1.63. [2]

This star has a stellar classification of B8/9III, [3] matching a B-type star that is in the giant stage. It has a high rate of spin with a projected rotational velocity of 130 km/s. [5] The star is radiating 485 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 11,540 K. [5]

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 e f g 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 Houk, N.; Smith-Moore, M. (1988), Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, vol. 4, Bibcode: 1988mcts.book.....H.
  4. ^ a b Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 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.
  5. ^ a b c d Paunzen, E.; et al. (December 2005), "An empirical temperature calibration for the ∆ a photometric system . I. The B-type stars", Astronomy and Astrophysics, 444 (3): 941–946, arXiv: astro-ph/0509049, Bibcode: 2005A&A...444..941P, doi: 10.1051/0004-6361:20053546, S2CID  119436374.
  6. ^ "42 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-08.
  7. ^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID  14878976.
From Wikipedia, the free encyclopedia
11 Canis Majoris
Observation data
Epoch J2000       Equinox J2000
Constellation Canis Major
Right ascension 06h 46m 51.09272s [1]
Declination −14° 25′ 33.5042″ [1]
Apparent magnitude (V) 5.28 [2]
Characteristics
Spectral type B8/9III [3]
B−V color index −0.024±0.004 [2]
Astrometry
Radial velocity (Rv)+15.0±4.2 [4] km/s
Proper motion (μ) RA: −2.853±0.344 [1]  mas/ yr
Dec.: +8.514±0.363 [1]  mas/ yr
Parallax (π)3.2263 ± 0.1847  mas [1]
Distance1,010 ± 60  ly
(310 ± 20  pc)
Absolute magnitude (MV)−1.63 [2]
Details
Luminosity485.12 [2]  L
Temperature11,540±181 [5]  K
Rotational velocity (v sin i)130 [5] km/s
Other designations
11 CMa, BD−14°1584, GC 8879, HD 49229, HIP 32492, HR 2504, SAO 151919 [6]
Database references
SIMBAD data

11 Canis Majoris is a single [7] star in the southern constellation of Canis Major, the eleventh entry in John Flamsteed's catalogue of stars in that constellation. It has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of 5.28. [2] The distance to this star is approximately 1,010  light years from the Sun based on parallax, [1] and it is drifting further away with a radial velocity of around +15 km/s. [4] It has an absolute magnitude of −1.63. [2]

This star has a stellar classification of B8/9III, [3] matching a B-type star that is in the giant stage. It has a high rate of spin with a projected rotational velocity of 130 km/s. [5] The star is radiating 485 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 11,540 K. [5]

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 e f g 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 Houk, N.; Smith-Moore, M. (1988), Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, vol. 4, Bibcode: 1988mcts.book.....H.
  4. ^ a b Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 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.
  5. ^ a b c d Paunzen, E.; et al. (December 2005), "An empirical temperature calibration for the ∆ a photometric system . I. The B-type stars", Astronomy and Astrophysics, 444 (3): 941–946, arXiv: astro-ph/0509049, Bibcode: 2005A&A...444..941P, doi: 10.1051/0004-6361:20053546, S2CID  119436374.
  6. ^ "42 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-08.
  7. ^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID  14878976.

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