NGC 6826 explained

NGC 6826
Type:Planetary
Epoch:J2000
Ra:[1]
Dist Ly:~2000
Appmag V:8.8
Size V:27 × 24[2]
Constellation:Cygnus
Radius Ly:0.22 x 0.20
Names:HD 186924, SAO 31951, Caldwell 15

NGC 6826 (also known as Caldwell 15) is a planetary nebula located in the constellation Cygnus. It is commonly referred to as the "Blinking Planetary", although many other nebulae exhibit such "blinking". When viewed through a small telescope, the brightness of the central star overwhelms the eye when viewed directly, obscuring the surrounding nebula. However, it can be viewed well using averted vision, which causes it to "blink" in and out of view as the observer's eye wanders.

A distinctive feature of this nebula are the two bright patches on either side, which are known as Fast Low-Ionization Emission Regions, or FLIERS. They appear to be relatively young, moving outwards at supersonic speeds.[3]

The central star of the planetary nebula is an O-type star with a spectral type of O6fp.[1]

See also

External links

Notes and References

  1. NGC 6826 . 2007-04-17.
  2. Web site: Stellar Scenes Image Collection . NGC 6826 . 2007-10-05 . 2016-03-03 . https://web.archive.org/web/20160303202504/http://www.ne.jp/asahi/stellar/scenes/object_e/ngc6826.htm . dead .
  3. Web site: astroimages.org . NGC 6826 : The Blinking Nebula . 2007-10-05.