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
Yep, but later
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.
The visual bandlight curve of LL Andromedae, adapted from Kato (2004), is shown. The main plot shows the decay from peak brightness, and the inset plot shows an average of the superhumps.[1]
LL Andromedae (often abbreviated to LL And) is a dwarf nova in the constellationAndromeda, discovered during an outburst in 1979. Its typical apparent visual magnitude is 19.4, but undergoes outbursts events when can reach a peak magnitude of 14.3.[1] Since this magnitude is reached during the most powerful outbursts, while less bright outbursts can occur, it is classified as a SU Ursae Majoris variable.[3]
YouTube Encyclopedic
1/5
Views:
12 389 684
1 427 569
5 286
759
17 091
Kepler Telescope Found New Planets Better Than Earth
The Andromeda-Milky Way Collision | Space Time
Find/see Great Andromeda Galaxy with your telescope (Messier 31 & Messier 32) - TOTS #1
Argentine Stroll/Tango part 2 of 3
3. The Search for other Earths and Life in the Universe
Transcription
Variability
The variability of LL Andromedae is similar to the WZ Sagittae type of dwarf novae. Those have a long outbursts cycle (they were observed only in 1979, 1994 and 2004)[5] and superhumps can be observed with a short periodic modulation. It was observed also a periodicity of 1.32 hours, which is attributed to the orbital period of the system. However, in comparison to WZ Sagittae, the outburst amplitude is small and the superoutbursts duration is short.[1]
System
Little is known about the components of LL Andromedae because it's a faint object; one of the two components is likely an accreting white dwarf like in all dwarf novae. A brown dwarf donor has been proposed, but the short periodicity of superhumps hints instead at the presence of a massive companion.[1]
This page was last edited on 23 February 2023, at 18:06