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Prime CV specimens-
U Gem
This variable is the typical star of its class and was the first to be discovered. J.R. Hind, an
English astronomer in charge of a private observatory in Regents Park, found a previously unlisted star in the constellation
Gemini to be nearly 9th magnitude on December 15, 1855.
SS Cyg
Since its discovery in 1896 by Louisa D. Wells of the Harvard College Observatory, SS Cygni
has undoubtedly been one of the most observed variable stars in the night sky.
SU UMa
Discovered in 1908 by L. Ceraski of Moscow, the variable SU Ursae Majoris is the prototype for
variables belonging to this subtype of dwarf novae.
Z Cam
Z Camelopardalis is the prototype star of a subclass of dwarf nova-type cataclysmic variables
especially known for their random standstills.
WZ Sge
WZ Sge - the prototype of the WZ Sge subclass of dwarf nova cataclysmic variables -
went into a rare outburst on July 23, 2001, captivating the attention of amateur and professional astronomers around the globe.
AM Her
The exotic star AM Herculis is the namesake of the “AM Her stars” or “polars”,
a unique class of cataclysmic variables in which the magnetic field of the primary star (white dwarf) completely dominates
the accretion flow of the system.
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