HD 111597

Last updated
HD 111597
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Centaurus [1]
Right ascension 12h 50m 41.16339s [2]
Declination −33° 59 57.6527 [2]
Apparent magnitude  (V)4.90 [1]
Characteristics
Spectral type B9V [3]
B−V color index −0.031±0.002 [1]
Astrometry
Radial velocity (Rv)+4.00±4.20 [1] km/s
Proper motion (μ)RA: −29.710 [2] mas/yr
Dec.: −13.778 [2] mas/yr
Parallax (π)7.9731±0.2191  mas [2]
Distance 410 ± 10  ly
(125 ± 3  pc)
Absolute magnitude  (MV)−0.53 [1]
Details
primary
Mass 4.3 [4]   M
Radius 4.3 [5]   R
Luminosity 169 [5]   L
Surface gravity (log g)3.58 [5]   cgs
Temperature 10,043 [5]   K
Rotational velocity (v sin i)230 [6]  km/s
Age 321 [7]   Myr
secondary
Mass 0.35 [4]   M
Other designations
p Cen, CD−33°8653, FK5 1331, HD 111597, HIP 62683, HR 4874, SAO 203863, CCDM J12507-3400, WDS J12507-3400A [8]
Database references
SIMBAD data

HD 111597 is a suspected astrometric binary [9] star system in the southern constellation of Centaurus. It has the Bayer designation p Centauri, while HD 111597 is the star's identifier from the Henry Draper catalogue . The system is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.90. [1] It is located at a distance of approximately 410  light years from the Sun based on parallax, [2] and has an absolute magnitude of −0.53. [1] The system is a probable member of the Sco OB2 association of co-moving stars. [10] The visible component is a B-type main-sequence star with a stellar classification of B9V. [3]

References

  1. 1 2 3 4 5 6 7 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. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211 . Bibcode:2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940 . S2CID   244398875. Gaia DR3 record for this source at VizieR.
  3. 1 2 Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 3. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode:1982mcts.book.....H.
  4. 1 2 Gratton, R.; Squicciarini, V.; Nascimbeni, V.; Janson, M.; Reffert, S.; Meyer, M.; Delorme, P.; Mamajek, E. E.; Bonavita, M.; Desidera, S.; Mesa, D.; Rigliaco, E.; d'Orazi, V.; Vigan, A.; Lazzoni, C.; Chauvin, G.; Langlois, M. (2023). "Multiples among B stars in the Scorpius-Centaurus association". Astronomy and Astrophysics. 678: A93. arXiv: 2308.09962 . Bibcode:2023A&A...678A..93G. doi:10.1051/0004-6361/202346806.
  5. 1 2 3 4 Stassun, Keivan G.; et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694 . Bibcode:2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467 .
  6. Balona, L. A.; Ozuyar, D. (2020). "Pulsation among TESS a and B stars and the Maia variables". Monthly Notices of the Royal Astronomical Society. 493 (4): 5871. arXiv: 2001.04497 . Bibcode:2020MNRAS.493.5871B. doi: 10.1093/mnras/staa670 .
  7. Gontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars". Astronomy Letters. 38 (11): 694–706. arXiv: 1606.09028 . Bibcode:2012AstL...38..694G. doi:10.1134/S1063773712110035. S2CID   119108982.
  8. "HD 111597". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-01-30.
  9. Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society . 389 (2): 869–879. arXiv: 0806.2878 . Bibcode:2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x . S2CID   14878976.
  10. Rizzuto, Aaron; et al. (October 2011). "Multidimensional Bayesian membership analysis of the Sco OB2 moving group". Monthly Notices of the Royal Astronomical Society. 416 (4): 3108–3117. arXiv: 1106.2857 . Bibcode:2011MNRAS.416.3108R. doi: 10.1111/j.1365-2966.2011.19256.x . S2CID   54510608.