To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
Languages
Recent
Show all languages
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

Cygnus OB7
Observation data (J2000.0 epoch)
ConstellationCygnus
Right ascension21h 08m 00s[1]
Declination47° 36′ 00″
Mean distance2,050 ly (630 pc[2])
Physical characteristics
See also: Stellar association, Moving groups

Cygnus OB7 is an OB association in the giant Cygnus molecular cloud complex, which also contains the star-forming regions Cygnus X, the North America Nebula and the Pelican Nebula. The Northern Coalsack Nebula of the Cygnus Rift lies in the foreground of this region. The molecular cloud has a large angular size of ~4° × 7°.[3]

References

  1. ^ "SIMBAD Astronomical Database". Results for Ass Cygnus OB7. Retrieved February 16, 2015.
  2. ^ Melnik, A. M.; Dambis, A. K. (2020). "Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions". Astrophysics and Space Science. 365 (7): 112. arXiv:2006.14649. Bibcode:2020Ap&SS.365..112M. doi:10.1007/s10509-020-03827-0. S2CID 220128144.
  3. ^ Dobashi, Kazuhito; Matsumoto, Tomoaki; Shimoikura, Tomomi; Saito, Hiro; Akisato, Ko; Ohashi, Kenjiro; Nakagomi, Keisuke (2014-11-24). "Colliding Filaments and a Massive Dense Core in the Cygnus Ob 7 Molecular Cloud". The Astrophysical Journal. American Astronomical Society. 797 (1): 58. arXiv:1411.0942. Bibcode:2014ApJ...797...58D. doi:10.1088/0004-637x/797/1/58. ISSN 1538-4357. S2CID 118369651.
This page was last edited on 8 October 2023, at 16:24
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.