411 REFERENCE · Wikipedia
12 Scorpii
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Star in the constellation Scorpius
c1 Scorpii other stars with this Bayer designation c Scorpii
12 Scorpii
J2000.0 J2000.0 Scorpius 16 12 16.039 −28 25 02.31 5.67 (5.79 + 7.9 + 8.13)
B9V1999MSS...C05....0H Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, Vol. 5 Michigan Spectral Survey 5 Houk, N. Swift, C. 1999 + K7.9XR? + F3V +0.01Catalogue of homogeneous data in the UBV photoelectric photometric system 1964 Astronomy and Astrophysics Supplement Series 34 1–49 Nicolet, B. 1978A&AS...34....1N −0.19
−0.2 1.8Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system Gontcharov, G. A. 2006 Astronomy Letters 32 11 759–771 2006AstL...32..759G 10.1134/S1063773706110065 1606.08053 119231169 −23.68 0.76 −42.44 0.69 10.75 0.80 +0.56Search for low-mass PMS companions around X-ray selected late B stars
Hubrig S. Le Mignant D.
North P. Krautter J.
Astronomy and Astrophysics 1
372 152–164 June 2001
10.1051/0004-6361:20010452 2001A&A...372..152H
astro-ph/0103201 17507782 .
12 Sco A 2.939 0.088 91 11,402 150
c1 Sco 12 Sco −28°11962 3226 145483 79399 6029 184217
12+Sco
12 Scorpii is a probable triple star system in the zodiac constellation of Scorpius, located about 300 light years away from the Sun. It has the Bayer designation c1 Scorpii; 12 Scorpii is the Flamsteed designation. This system is faintly visible to the naked eye with a combined apparent visual magnitude of 5.67. It is a probable (82% chance) member of the Sco OB2 moving group.
The magnitude 5.79 primary component is a B-type main-sequence star with a stellar classification of B9V. This star is 150 million years old with three times the mass of the Sun. It is radiating 91 times the Sun's luminosity from its photosphere at an effective temperature of 11,402 K. At an angular separation of 0.20 arcsecond is a K7.9 type secondary companion, a possible X-ray source. The third component is an F-type main-sequence star of class F3V and magnitude 8.13, located at a separation of 3.84 arcsecond.
References
2 Sco 2019-03-23
Validation of the new Hipparcos reduction http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...474..653VFUL van Leeuwen F. Astronomy and Astrophysics 474 2 653–664 2007 0708.1752 2007A&A...474..653V 10.1051/0004-6361:20078357 free 18759600 Vizier catalog entry
Rizzuto Aaron
Ireland Michael Robertson J. G.
Multidimensional Bayesian membership analysis of the Sco OB2 moving group
Monthly Notices of the Royal Astronomical Society
October 2011 416 4 3108–3117
2011MNRAS.416.3108R 1106.2857
10.1111/j.1365-2966.2011.19256.x free
54510608
Eggleton P. P. Tokovinin A. A.
A catalogue of multiplicity among bright stellar systems
Monthly Notices of the Royal Astronomical Society
389 2 869–879 September 2008
2008MNRAS.389..869E 0806.2878
10.1111/j.1365-2966.2008.13596.x free 14878976
Category:B9V stars
Category:F-type main-sequence stars
Category:Scorpius
Scorpii, 12
Scorpii, c1
Category:Durchmusterung objects
145483
079399
6029