astro.wikisort.org - StarSigma Arae (σ Ara, σ Arae) is the Bayer designation for a star in the southern constellation of Ara. It is visible to the naked eye with an apparent visual magnitude of +4.575.[2] The distance to this star, based upon an annual parallax shift of 8.62 mas,[1] is around 380 light-years (120 parsecs).
Star in the constellation Ara
Sigma Arae
The location of σ Arae (circled) |
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Ara |
Right ascension |
17h 35m 39.58957s[1] |
Declination |
–46° 30′ 20.4618″[1] |
Apparent magnitude (V) |
+4.575[2] |
Characteristics |
Spectral type |
A0 V[3] |
U−B color index |
–0.064[2] |
B−V color index |
–0.027[2] |
Astrometry |
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Proper motion (μ) | RA: –25.78[1] mas/yr Dec.: –38.30[1] mas/yr |
Parallax (π) | 8.62 ± 0.26 mas[1] |
Distance | 380 ± 10 ly (116 ± 3 pc) |
Absolute magnitude (MV) | 1.40[4] |
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Details |
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Luminosity (bolometric) | 26.4[4] L☉ |
Temperature | 9,790[4] K |
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Other designations |
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CD–46 11661, HD 159217, HIP 86092, HR 6537, SAO 228162. [5] |
Database references |
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SIMBAD | data |
This is an A-type main sequence star with a stellar classification of A0 V.[3] Unusually for an A-type star, X-ray emissions with a luminosity of 4.6 × 1029 erg s−1 have been detected from Sigma Arae. Normally this is explained by the presence of a lower mass orbiting companion star. However, such a scenario does not appear to hold true for this star. Instead, the signature of a surface magnetic field has been detected with a strength of roughly 128 ± 73 Gauss, indicating the source of the X-rays may be surface magnetic activity.[6]
References
- 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.
- Cousins, A. W. J. (1973), "Revised zero points and UBV photometry of stars in the Harvard E and F regions", Memoirs of the Royal Astronomical Society, 77: 223–236, Bibcode:1973MmRAS..77..223C.
- Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
- Neff, James E.; Simon, Theodore (September 2008), "O VI Observations of the Onset of Convection Zones in Main-Sequence A Stars", The Astrophysical Journal, 685 (1): 478–488, arXiv:0805.4459, Bibcode:2008ApJ...685..478N, doi:10.1086/590423, S2CID 8607533
- "* sig Ara". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-08-02.
{{cite web}}
: CS1 maint: postscript (link) - Schröder, C.; Hubrig, S.; Schmitt, J. H. M. M. (June 2008), "Magnetic fields in A-type stars associated with X-ray emission", Astronomy and Astrophysics, 484 (2): 479–486, Bibcode:2008A&A...484..479S, doi:10.1051/0004-6361:20078963
External links
Constellation of Ara |
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Stars | |
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Star clusters | |
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Nebulae | |
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