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46 Aquilae

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(Redirected from 46 Aql) Star in the constellation Aquila
46 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19 42 12.81242
Declination 12° 11′ 35.7382″
Apparent magnitude (V) 6.33
Characteristics
Spectral type B9III
U−B color index −0.42
B−V color index −0.077±0.004
Astrometry
Radial velocity (Rv)−24.7±1.6 km/s
Proper motion (μ) RA: −0.495 mas/yr
Dec.: −8.147 mas/yr
Parallax (π)3.9251 ± 0.0579 mas
Distance830 ± 10 ly
(255 ± 4 pc)
Absolute magnitude (MV)−0.32
Details
Luminosity179.50 L
Surface gravity (log g)3.7 cgs
Temperature12,900 K
Metallicity 0.50 dex
Rotational velocity (v sin i)1.0±0.5 km/s
Other designations
46 Aql, BD+11° 3954, GC 27263, HD 186122, HIP 96931, HR 7493, SAO 105156
Database references
SIMBADdata

46 Aquilae is a star in the constellation of Aquila, located to the north of Tarazed (γ Aquilae). 46 Aquilae is its Flamsteed designation. It is a dim, blue-white hued star that is a challenge to view with the naked eye, having an apparent visual magnitude of 6.33. This object is located approximately 830 light years from the Sun, based on parallax. It is moving closer to the Earth with a heliocentric radial velocity of −25 km/s.

This body has a stellar classification of B9 III, matching a late B-type giant star. It is a chemically peculiar star of a weak Mercury-Manganese type (CP3), and is the most chromium–deficient star known. The star may possess a magnetic field with a strength greater than 2 kG. It is radiating 180 times the luminosity of the Sun from its photosphere at an effective temperature of 12,900 K.

References

  1. ^ 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. ^ 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. ^ "46 Aql". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-06-05.
  4. Crawford, D. L. (February 1963), "U, b, v, and Hβ Photometry for the Bright B8- and B9-TYPE Stars", Astrophysical Journal, 137: 530, Bibcode:1963ApJ...137..530C, doi:10.1086/147526.
  5. ^ Bailey, J. D.; Landstreet, J. D. (2013). "Abundances determined using Si ii and Si iii in B-type stars: Evidence for stratification". Astronomy & Astrophysics. 551: A30. arXiv:1301.3050. Bibcode:2013A&A...551A..30B. doi:10.1051/0004-6361/201220671. S2CID 59291051.
  6. Smith, K. C.; Dworetsky, M. M. (1993), "Elemental Abundances in Normal Late B-Stars and Hgmn-Stars from Co-Added IUE Spectra - Part One - Iron Peak Elements", Astronomy and Astrophysics, 274 (2): 335, Bibcode:1993A&A...274..335S.
  7. Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819.
  8. Ghazaryan, S.; et al. (November 2018), "New catalogue of chemically peculiar stars, and statistical analysis", Monthly Notices of the Royal Astronomical Society, 480 (3): 2953–2962, arXiv:1807.06902, Bibcode:2018MNRAS.480.2953G, doi:10.1093/mnras/sty1912.
  9. Savanov, I.; Hubrig, S. (October 2003), "Vertical distribution of chromium in the atmospheres of HgMn stars", Astronomy and Astrophysics, 410: 299–305, arXiv:astro-ph/0309562, Bibcode:2003A&A...410..299S, doi:10.1051/0004-6361:20031270, S2CID 14487812.
  10. Hubrig, S.; et al. (2001), "Magnetic Field Diagnosis in HgMn Stars", in Mathys, G.; Solanki, S. K.; Wickramasinghe, D. T. (eds.), Magnetic Fields Across the Hertzsprung-Russell Diagram, ASP Conference Proceedings, vol. 248, San Francisco: Astronomical Society of the Pacific, p. 387, Bibcode:2001ASPC..248..387H, ISBN 1-58381-088-9.
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