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12 Lyncis

Star in the constellation Lynx


Star in the constellation Lynx

| b-v= | u-b=+0.08 | b-v=+0.08 12 Lyncis, abbreviated 12 Lyn, is a triple star system in the constellation Lynx. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.87. When seen through a telescope, it can be separated into three stars: two components with magnitudes 5.4 and 6.0 that lie at an angular separation by 1.8″ (as of 1992) and a yellow-hued star of magnitude 7.2 at a separation of 8.6″ (as of 1990). The orbit of the two brighter stars is not known with certainty, but appears to have a period of somewhere around 700 to 900 years. The pair have a projected separation of . Parallax indicates the system is light years distant from Earth.

References

| display-authors=1 | last1=Mason | first1=Brian D.

References

  1. van Leeuwen, F.. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics.
  2. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters.
  3. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory.
  4. Gontcharov, G. A.. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters.
  5. "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory.
  6. (January 2009). "An analysis of v sin (i) correlations in early-type binaries". [[Monthly Notices of the Royal Astronomical Society]].
  7. "* 12 Lyn".
  8. (September 2008). "A catalogue of multiplicity among bright stellar systems". [[Monthly Notices of the Royal Astronomical Society]].
  9. Monks, Neale. (2010). "Go-To Telescopes Under Suburban Skies". [[Springer Science & Business Media]].
  10. (2012). "Dynamical Masses of a Selected Sample of Orbital Binaries". Astronomy and Astrophysics.
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