- Beta
Canum Venaticorum (β
Canum Venaticorum,
abbreviated Beta CVn, β CVn), also
named Chara /ˈkɛərə/, is a G-type main-sequence star in the
northern constellation...
- /ˌkɔːr ˈkærəlaɪ/ is a
binary star
designated Alpha Canum Venaticorum or α
Canum Venaticorum. The
International Astronomical Union uses the name "Cor Caroli"...
-
Canum Venaticorum (CVn); however, 1 CVn
turned out to be in Ursa Major, 13 CVn was in Coma Berenices, and 22 CVn did not exist.
Alpha Canum Venaticorum, also...
-
derived from
adding the
magnitudes of Alpha2
Canum Venaticorum (2.88) and Alpha1
Canum Venaticorum (5.60) as per the formula: 2.79 ≈ − 2.5 log 10 (...
- La
Superba (Y CVn, Y
Canum Venaticorum) is a
strikingly red
giant star in the
constellation Canes Venatici. It is
faintly visible to the
naked eye, and...
- An RS
Canum Venaticorum variable is a type of
variable star. The
variable type
consists of
close binary stars having active chromospheres which can cause...
- An AM
Canum Venaticorum star (AM CVn star), is a rare type of
cataclysmic variable star
named after their type star, AM
Canum Venaticorum. In
these hot...
- An Alpha2
Canum Venaticorum variable (or α2 CVn variable) is a type of
variable star.
These stars are
chemically peculiar main
sequence stars of spectral...
- DG
Canum Venaticorum is a
variable binary star
system in the
northern constellation of
Canes Venatici. As of 2009, the pair have an
angular separation...
-
Venaticorum is a
binary star
system in the
northern constellation of
Canes Venatici. It
serves as the
prototype to the
class of RS
Canum Venaticorum variables...
