Star in the constellation of Antlia
HD 86267 , also known asHR 3932 , is a solitary[ 14] orange-huedstar located in the southernconstellation Antlia . It has anapparent magnitude of 5.82,[ 2] allowing it to be faintly seen with thenaked eye .Parallax measurements place it a distance of 514light years [ 1] and it is currently receding with a heliocentricradial velocity of 3.7 km/s .[ 5]
HD 86267 has astellar classification of K1 III,[ 3] indicating that it is ared giant . At present it has 1.73 times themass of the Sun [ 7] but has expanded to 19.7 times its girth.[ 8] It shines with aluminosity of 158 L ☉ from its enlargedphotosphere at aneffective temperature of 4,430 K .[ 7] It is a member of the old disk population, having ametallicity 71% that of theSun .[ 10] The value means that it is metal deficient. Its currentrotation rate is too low to be measured accurately.[ 11]
^a b c d e f 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 atVizieR .^a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics .355 :L27 – L30 .Bibcode :2000A&A...355L..27H .ISSN 0004-6361 . ^a b Houk, N. (1982).Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations −40° to −26° .Bibcode :1982mcts.book.....H . ^ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory .4 :99– 110.Bibcode :1966CoLPL...4...99J . ^a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".Astronomy Letters .32 (11):759– 771.arXiv :1606.08053 .Bibcode :2006AstL...32..759G .doi :10.1134/S1063773706110065 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119231169 . ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters .38 (5):331– 346.arXiv :1108.4971 .Bibcode :2012AstL...38..331A .doi :10.1134/S1063773712050015 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 255204555 . ^a b c d e Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020)."Lithium in red giant stars: Constraining non-standard mixing with large surveys in theGaia era" .Astronomy & Astrophysics .633 : A34.arXiv :1910.12732 .Bibcode :2020A&A...633A..34C .doi :10.1051/0004-6361/201936360 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Stassun, Keivan G.; et al. (9 September 2019)."The RevisedTESS 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 .eISSN 1538-3881 . ^ Anders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia DR2 stars brighter thanG = 18" .Astronomy & Astrophysics .628 : A94.arXiv :1904.11302 .Bibcode :2019A&A...628A..94A .doi :10.1051/0004-6361/201935765 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Eggen, Olin J. (April 1989)."Large and kinematically unbiased samples of G- and K-type stars. IV - Evolved stars of the old disk population" .Publications of the Astronomical Society of the Pacific .101 : 366.Bibcode :1989PASP..101..366E .doi :10.1086/132442 .eISSN 1538-3873 .ISSN 0004-6280 . ^a b De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014)."A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆" .Astronomy & Astrophysics .561 : A126.arXiv :1312.3474 .Bibcode :2014A&A...561A.126D .doi :10.1051/0004-6361/201220762 .ISSN 0004-6361 . ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas".Resultados del Observatorio Nacional Argentino .1 .Bibcode :1879RNAO....1.....G . ^ "HR 3932" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved4 August 2022 .^ Eggleton, P. P.; Tokovinin, A. A. (11 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 .eISSN 1365-2966 .ISSN 0035-8711 .