Jump to content

Banner.jpg.b83b14cd4142fe10848741bb2a14c66b.jpg

NGC7822 / Cederblad 214


Avdhoeven

Recommended Posts

 

NGC 7822 is a young star forming complex in the constellation of Cepheus. The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59. The complex is believed to be some 800-1000 pc distant, with the younger components aged no more than a few million years. The complex also includes one of the hottest stars discovered within 1 kpc of the Sun, namely BD+66 1673, which is an eclipsing binary system consisting of an O5V that exhibits a surface temperature of nearly 45000 K and a luminosity ~100000 times that of the Sun. The star is one of the primary sources illuminating the nebula and shaping the complex’s famed pillars of creation-type formations, the elephant trunks.

This image consists of 52 exposures of 900s each, totaling to 13 hours.

Telescope: TMB92SS
Camera: QSI583ws

Exposures:

25x900s Ha (5nm)

8x900s OIII (3nm)

19x900s SII (5nm)

 

29568783643_37290df5d9_b.jpg

NGC 7822 widefield by Andre van der Hoeven, on Flickr

Link to comment
Share on other sites

Archived

This topic is now archived and is closed to further replies.

  • Recently Browsing   0 members

    • No registered users viewing this page.
×
×
  • Create New...

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue. By using this site, you agree to our Terms of Use.