Binary star in the constellation Aquarius
Psi3 Aquarii ,Latinized from ψ3 Aquarii, is theBayer designation for a visualbinary star [ 9] system in theconstellation ofAquarius . It has anapparent visual magnitude of 4.98,[ 2] which is bright enough to be seen with the naked eye.Parallax measurements give a distance estimate of roughly 262light-years (80parsecs ).[ 1]
The main component of this system is anA-type main sequence star with astellar classification of A0 V.[ 3] Its companion is an 11th magnitude star 1.5arcseconds from the primary.[ 10] This system is anX-ray source with a luminosity of8.34 × 1029 erg s−1 . This radiation most likely comes from the companion star.[ 9]
^a b c d e f van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics ,474 (2):653– 664,arXiv :0708.1752 ,Bibcode :2007A&A...474..653V ,doi :10.1051/0004-6361:20078357 ,S2CID 18759600 . ^a b c Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",Communications of the Lunar and Planetary Laboratory ,4 (99): 99,Bibcode :1966CoLPL...4...99J . ^a b 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 . ^ Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities",Carnegie Institute Washington D.C. Publication , Washington: Carnegie Institution of Washington,Bibcode :1953GCRV..C......0W . ^a b 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 . ^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics",Astronomy and Astrophysics ,367 (2):521– 524,arXiv :astro-ph/0012289 ,Bibcode :2001A&A...367..521P ,doi :10.1051/0004-6361:20000451 ,S2CID 425754 . ^ Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions",Astronomy and Astrophysics ,463 (2):671– 682,arXiv :astro-ph/0610785 ,Bibcode :2007A&A...463..671R ,doi :10.1051/0004-6361:20065224 ,S2CID 18475298 . ^ "* psi03 Aqr" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved2012-07-05 .^a b Schröder, C.; Schmitt, J. H. M. M. (November 2007), "X-ray emission from A-type stars",Astronomy and Astrophysics ,475 (2):677– 684,Bibcode :2007A&A...475..677S ,doi :10.1051/0004-6361:20077429 . ^ 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 .