Chú thích Tinh vân Mắt Mèo

  1. Distance × sin(diameter_angle / 2) = 0,2 ly. radius
  2. 9.8B apparent magnitude – 5×{log(1,0 ± 0,3 kpc distance) − 1} = −0,2+0,8
    −0,6B absolute magnitude
  1. 1 2 3 4 5 6 7 (SIMBAD 2006)
  2. 1 2 (Reed và đồng nghiệp 1999)
  3. 1 2 3 “HST Measurements of the Expansion of NGC Parallax Distance and Nebular Evolution” (PDF). Reed D.S., Balick B., Hajian A.R. et al (1999). Truy cập ngày 31 tháng 8 năm 2006. 
  4. 1 2 3 Wesson R., Liu X.-W. (2004), "Physical conditions in the planetary nebula NGC 6543", Monthly Notices of the Royal Astronomical Society, vol. 351, p.1026
  5. Bianchi L., Cerrato S., Grewing M. (1986), "Mass loss from central stars of planetary nebulae - The nucleus of NGC 6543", Astronomy and Astrophysics, vol. 169, p.227
  6. Hora J.L., Latter W.B., Allen L.E. et al (2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae", Astrophysical Journal Supplement Series, vol. 154, p.296
  7. Guerrero M.A., Chu Y-H., Gruendl R.A., (2001), "The Enigmatic X-Ray Point Sources at the Central Stars of NGC 6543 and NGC 7293", Astrophysical Journal, vol. 553, p.55
  8. Hyung S., Aller L.H., Feibelman W.A. et al (2000), "The optical spectrum of the planetary nebula NGC 6543", Monthly Notices of the Royal Astronomical Society, vol. 318, p.77
  9. Balick B., Preston H.L. (1987), "A wind-blown bubble model for NGC 6543", Astronomical Journal, vol. 94, p.958
  10. Miranda L.F., Solf J. (1992), "Long-slit spectroscopy of the planetary nebula NGC 6543 - Collimated bipolar ejections from a precessing central source?", Astronomy and Astrophysics, vol. 260, p.397
  11. Balick B., Wilson J., Hajian A.R. (2001), "NGC 6543: The Rings Around the Cat's Eye", Astronomical Journal, vol. 121, p.354