Top Qs
Timeline
Chat
Perspective
Z Camelopardalis
Star in the constellation Camelopardalis From Wikipedia, the free encyclopedia
Remove ads
Z Camelopardalis (Z Cam) is a cataclysmic variable star system in the northern constellation of Camelopardalis. It has an apparent visual magnitude which varies between 9.8 and 14.5. This system is the prototype star for the family of Z Camelopardalis variable stars: dwarf novae with standstills at a brightness intermediate between their maxima and minima.[3] It may have been the "guest star" that was recorded by Chinese astrologers in the autumn of 77 BCE,[6] but a 2024 study argues that this guest star was likely a comet, while one observed in 369 CE may have been Z Camelopardalis.[7]
Z Camelopardalis was discovered photographically in 1904 by Henry Park Hollis during work for the Astrographic Catalogue.[8] It is surrounded by an extensive shell thought to have been ejected in a nova explosion,[9] the largest known of its type. The size and expansion of this shell sets a firm lower limit since the last eruption of at least 220 years.[6]
Remove ads
Gallery
- Z Camelopardalis light curve showing a characteristic standstill interrupting the otherwise regular eruptions
- Gas shell Around Z Camelopardalis
- Z Camelopardalis in ultraviolet
References
External links
Wikiwand - on
Seamless Wikipedia browsing. On steroids.
Remove ads