Star in the constellation Pictor
AE Pictoris is an eclipsing binary [ 6] star system in the southern constellation of Pictor . This dim, blue-white hued point of light is just barely visible to the naked eye; it has an apparent visual magnitude of 6.09, which drops to magnitude 6.14 during an eclipse.[ 13] The system is located around 1,430 light years away from the Sun based on parallax ,[ 2] and it is receding with a radial velocity of 34 km/s.[ 14]
This is a spectroscopic binary system with an orbital period of 2.97 days and an eccentricity of 0.10. The minimum value of the semimajor axis for the pair is 4.8 Gm (6.9 R ☉ ).[ 7] The secondary star was only recently (in 2023) detected, making it a double-lined spectroscopic binary.[ 10] It is classed as a probable eclipsing binary variable (EB:), but with some uncertainty regarding the specific type.[ 6] This is a candidate runaway star system, having a peculiar velocity of 24.9+4.9 −5.1 km/s relative to its neighbors.[ 8] The visible component is a B-type main-sequence star with a stellar classification of B3V.[ 4] it is 28 million years old with seven[ 8] times the mass of the Sun . The star is radiating 2,569 times the luminosity of the Sun from its photosphere at an effective temperature of 18,700 K.[ 9]
References
^ Pedersen, May G.; Chowdhury, Sowgata; Johnston, Cole; Bowman, Dominic M.; Aerts, Conny; Handler, Gerald; De Cat, Peter; Neiner, Coralie; David-Uraz, Alexandre; Buzasi, Derek; Tkachenko, Andrew; Simón-Díaz, Sergio; Moravveji, Ehsan; Sikora, James; Mirouh, Giovanni M.; Lovekin, Catherine C.; Cantiello, Matteo; Daszyńska-Daszkiewicz, Jadwiga; Pigulski, Andrzej; Vanderspek, Roland K.; Ricker, George R. (February 2019). "Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample" . The Astrophysical Journal Letters . 872 (1): L9. arXiv :1901.07576 . Bibcode :2019ApJ...872L...9P . doi :10.3847/2041-8213/ab01e1 .
^ 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 .
^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000), "The Tycho-2 catalogue of the 2.5 million brightest stars", Astronomy and Astrophysics , 355 : L27, Bibcode :2000A&A...355L..27H .
^ a b Hiltner, W. A.; et al. (July 1969), "MK Spectral Types for Bright Southern OB Stars", Astrophysical Journal , 157 : 313– 326, Bibcode :1969ApJ...157..313H , doi :10.1086/150069 .
^ a b c 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 .
^ a b c Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports , 5.1, 61 (1): 80– 88, Bibcode :2017ARep...61...80S , doi :10.1134/S1063772917010085 , S2CID 125853869 .
^ a b Sahade, J.; Landi Dessy, J. (January 1950), "The Spectroscopic Binary CPD -61°669", Astrophysical Journal , 111 : 191, Bibcode :1950ApJ...111..191S , doi :10.1086/145251 .
^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society , 410 (1): 190– 200, arXiv :1007.4883 , Bibcode :2011MNRAS.410..190T , doi :10.1111/j.1365-2966.2010.17434.x , S2CID 118629873 .
^ a b Hohle, M. M.; et al. (2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten , 331 (4): 349, arXiv :1003.2335 , Bibcode :2010AN....331..349H , doi :10.1002/asna.200911355 , S2CID 111387483 .
^ a b c d e f g Kovalev, Mikhail; Straumit, Ilya (2023). "Application of the binary spectral model to high-resolution spectra. First estimation of the fundamental parameters for HD 20784" . Monthly Notices of the Royal Astronomical Society . 523 (3): 3741– 3748. arXiv :2210.00863 . Bibcode :2023MNRAS.523.3741K . doi :10.1093/mnras/stad1667 .
^ Barraza, L. F.; Gomes, R. L.; Messias, Y. S.; Leão, I. C.; Almeida, L. A.; Janot-Pacheco, E.; Brito, A. C.; Brito, F. A. C.; Santana, J. V.; Gonçalves, N. S.; Das Chagas, M. L.; Teixeira, M. A.; De Medeiros, J. R.; Canto Martins, B. L. (2022). "Rotation Signature of TESS B-type Stars. A Comprehensive Analysis" . The Astrophysical Journal . 924 (2): 117. arXiv :2202.01022 . Bibcode :2022ApJ...924..117B . doi :10.3847/1538-4357/ac3335 . S2CID 246030494 .
^ "AE Pic" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-08-03 .
^ Avvakumova, E. A.; et al. (October 2013), "Eclipsing variables: Catalogue and classification", Astronomische Nachrichten , 334 (8): 860, Bibcode :2013AN....334..860A , doi :10.1002/asna.201311942 , hdl :10995/27061 .
^ Wilson, Ralph Elmer (1953), "General catalogue of stellar radial velocities", Carnegie Institute Washington D.C. Publication , Bibcode :1953GCRV..C......0W .
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