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Mu Pictoris

From Wikipedia, the free encyclopedia
Variable star in the constellation Pictor
Mu Pictoris
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationPictor
Right ascension06h 31m 58.31021s[1]
Declination−58° 45′ 13.8117″[1]
Apparent magnitude (V)5.69[2](5.71 + 9.43)[3]
Characteristics
Spectral typeB9 Ve[4] or B9 IVn + A8 V:p?[5]
U−Bcolor index−0.17[2]
B−Vcolor index−0.06[2]
Astrometry
Radial velocity (Rv)+0.40±1.00[6] km/s
Proper motion (μ)RA: −1.34[1]mas/yr
Dec.: +1.77[1]mas/yr
Parallax (π)4.31±0.38 mas[1]
Distance760 ± 70 ly
(230 ± 20 pc)
Absolute magnitude (MV)0.20/3.75[7]
Details
μ Pic A
Mass3.60±0.09[8] M
Luminosity355[8] L
Temperature10,568[8] K
Rotational velocity (v sin i)228[8] km/s
Other designations
μ Pic,CPD−58° 722,HD 46860,HIP 31137,HR 2412,SAO 234564[9]
Database references
SIMBADdata

μ Pictoris, Latinised asMu Pictoris, is abinary star[3] system in the southernconstellationPictor. It is bright enough to be dimly visible to the naked eye, having a combinedapparent visual magnitude of 5.69.[2] Based upon an annualparallax shift of 4.31 mas as seen from Earth,[1] the system is located roughly 760 light years distant from theSun. As of 2010, the pair have anangular separation of 2.46 arc seconds along aposition angle of 221°.[4]

The primary, designated component A, is a blue-white star with a visual magnitude of 5.71[3] and astellar classification of B9 Ve[4] or B9 IVn.[5] The first classification suggests is aB-type main-sequence star, with the 'e' suffix indicating aBe star. The second may instead indicate a somewhat moreevolvedB-type star that is spinning rapidly, resulting in "nebulous"absorption lines.Photometrically, it shows a pulsation period of 0.397 days, which is likely the same as the rotation period.[10]

The secondary companion, component B, is a white-hued star of magnitude 9.43[3] with a classification of A8 V:p?.[5] This indicates it is anA-type main-sequence star, with the 'p?' suffix suggesting it may bechemically peculiar while the ':' notation says there is some uncertainty about the general classification.

References

[edit]
  1. ^abcdefvan Leeuwen, F. (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.
  2. ^abcdHurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles",Monthly Notes of the Astronomical Society of Southern Africa,34: 7,Bibcode:1975MNSSA..34....7H.
  3. ^abcdEggleton, 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.
  4. ^abcOudmaijer, René D.; Parr, Andrew M. (July 2010), "The binary fraction and mass ratio of Be and B stars: a comparative Very Large Telescope/NACO study",Monthly Notices of the Royal Astronomical Society,405 (4):2439–2446,arXiv:1003.0618,Bibcode:2010MNRAS.405.2439O,doi:10.1111/j.1365-2966.2010.16609.x,S2CID 119209332.
  5. ^abcCorbally, C. J. (1984), "Close visual binaries. I - MK classifications",Astrophysical Journal Supplement Series,55: 657,Bibcode:1984ApJS...55..657C,doi:10.1086/190973.
  6. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  7. ^Corbally, C. J. (December 1984), "Close visual binaries. III - Parameters and evolutionary status",Astronomical Journal,89:1887–1896,Bibcode:1984AJ.....89.1887C,doi:10.1086/113700.
  8. ^abcdZorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  9. ^"mu. Pic".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-08-08.{{cite web}}: CS1 maint: postscript (link)
  10. ^Balona, L. A. (December 1995), "Tests of the Pulsation and Starspot Models for the Periodic Be-Stars",Monthly Notices of the Royal Astronomical Society,277 (4): 1547,Bibcode:1995MNRAS.277.1547B,doi:10.1093/mnras/277.4.1547.
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