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.

How to transfigure the Wikipedia

Would you like Wikipedia to always look as professional and up-to-date? We have created a browser extension. It will enhance any encyclopedic page you visit with the magic of the WIKI 2 technology.

Try it — you can delete it anytime.

Install in 5 seconds
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
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
Great Wikipedia has got greater.
.
Leo
Newton
Brights
Milds

UGCA 86

From Wikipedia, the free encyclopedia

UGCA 86
UGCA 86 as taken by Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationCamelopardalis
Right ascension03h 59m 50.5s[1]
Declination+67° 08′ 37″[1]
Redshift67 ± 4 km/s[1]
Distance9.72 ± 0.91 Mly (2.98 ± 0.28 Mpc)[2]
Apparent magnitude (V)13.5[1]
Absolute magnitude (V)−17.0[3]
Characteristics
TypeIm[1]
Apparent size (V)5.0′ × 3.0′ [1]
Other designations
PGC 14241[1]

UGCA 86 is a Magellanic spiral galaxy. It was first thought to be part of the Local Group, but after the brightest stars in the galaxy were observed, it became clear that it was located in the IC 342/Maffei Group.[4] UGCA 86 is thought to be a satellite galaxy of IC 342, however the separation between the two galaxies is over 50% larger than the distance between the Milky Way and the Magellanic Clouds.[3]

References

  1. ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for UGCA 86. Retrieved 2006-11-30.
  2. ^ Karachentsev, Igor D.; Makarova, Lidia N.; Brent Tully, R.; Anand, Gagandeep S.; Rizzi, Luca; Shaya, Edward J.; Afanasiev, Viktor L. (2020). "KKH 22, the first dwarf spheroidal satellite of IC 342". Astronomy & Astrophysics. 638: A111. arXiv:2005.03132. Bibcode:2020A&A...638A.111K. doi:10.1051/0004-6361/202037993. S2CID 218538458.
  3. ^ a b Stil, J. M.; Gray, A. D.; Harnett, J. I. (2005). "H I Distribution and Kinematics of UGCA 86". The Astrophysical Journal. 625 (1): 130–142. arXiv:astro-ph/0408134. Bibcode:2005ApJ...625..130S. doi:10.1086/424962. S2CID 6461207.
  4. ^ I. D. Karachentsev (2005). "The Local Group and Other Neighboring Galaxy Groups". Astronomical Journal. 129 (1): 178–188. arXiv:astro-ph/0410065. Bibcode:2005AJ....129..178K. doi:10.1086/426368. S2CID 119385141.

External links


This page was last edited on 29 June 2023, at 05:38
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.
Contact WIKI 2
Introduction
Terms of Service
Privacy Policy