Astronomy:HD 16004

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Short description: Cmeically peculiar B-type star in the constellation Andromeda
HD 16004
Observation data
Equinox J2000.0]] (ICRS)
Constellation Andromeda
Right ascension  02h 35m 27.90126s[1]
Declination +39° 39′ 51.7705″[1]
Apparent magnitude (V) 6.26[2]
Characteristics
Spectral type B9.5 III HgMn[2]
U−B color index −0.33[2]
B−V color index −0.30[2]
Astrometry
Radial velocity (Rv)−6.8±1.1[3] km/s
Proper motion (μ) RA: +16.659[1] mas/yr
Dec.: −34.296[1] mas/yr
Parallax (π)4.9384 ± 0.1650[1] mas
Distance660 ± 20 ly
(202 ± 7 pc)
Absolute magnitude (MV)−0.36[4]
Details
Mass2.88[5] M☉
Radius3.274[6] R☉
Luminosity158[6] L☉
Surface gravity (log g)3.8[5] cgs
Temperature10,809[5] K
Metallicity [Fe/H]−0.17[5] dex
Rotational velocity (v sin i)30[7] km/s
Age162[8] Myr
Other designations
BD+39°573, GC 3093, HD 16004, HIP 12057, HR 746, SAO 55680, WDS J02355+3940A[9]
Database references
SIMBADdata

HD 16004 is blue-white hued star in the northern constellation of Andromeda. It is a challenge to see with the naked eye even under good viewing conditions, having an apparent visual magnitude of 6.26.[2] Located approximately 660 light-years (202 parsecs) away from the Sun based on parallax, it is drifting closer with a heliocentric radial velocity of −7 km/s.[3]

This is a chemically peculiar mercury-manganese star[10] with a stellar classification of B9.5 III HgMn.[2] It is an estimated 162 million years old and is spinning with a projected rotational velocity of 30 km/s.[7] The star is radiating 158 times the luminosity of the Sun from its photosphere at an effective temperature of 10,809 K.

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Jaschek, M. et al. (1980). "The absolute magnitude of the Hg-Mn stars". Astronomy and Astrophysics 81: 142. Bibcode: 1980A&A....81..142J. 
  3. ↑ 3.0 3.1 Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G. 
  4. ↑ Westin, T. N. G. (1985). "The local system of early type stars - Spatial extent and kinematics". Astronomy and Astrophysics Supplement Series 60: 99–134. Bibcode: 1985A&AS...60...99W. 
  5. ↑ 5.0 5.1 5.2 5.3 Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A. et al. (2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics 628: A94. doi:10.1051/0004-6361/201935765. Bibcode: 2019A&A...628A..94A. 
  6. ↑ 6.0 6.1 McDonald, I. et al. (2017). "Fundamental parameters and infrared excesses of Hipparcos stars". Monthly Notices of the Royal Astronomical Society 471 (1): 770–791. doi:10.1093/mnras/stx1433. Bibcode: 2017MNRAS.471..770M. 
  7. ↑ 7.0 7.1 Abt, Helmut A. et al. (2002). "Rotational Velocities of B Stars". The Astrophysical Journal 573 (1): 359–365. doi:10.1086/340590. Bibcode: 2002ApJ...573..359A. 
  8. ↑ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters 38 (12): 771–782. doi:10.1134/S1063773712120031. Bibcode: 2012AstL...38..771G. 
  9. ↑ "HD 16004". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+16004. 
  10. ↑ Renson, P.; Manfroid, J. (2009). "Catalogue of Ap, HgMn and Am stars". Astronomy and Astrophysics 498 (3): 961. doi:10.1051/0004-6361/200810788. Bibcode: 2009A&A...498..961R. 



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