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5 canum venaticorum es una gigante amarilla de tipo espectral g6iii.
5 canum venaticorum is a yellow g-type giant with an apparent magnitude of +4.76.

las variables alfa2 canum venaticorum son estrellas variables de la secuencia principal de tipo espectral b8p a a7p.
these stars are chemically peculiar main sequence stars of spectral class b8p to a7p.

* ε ursae minoris, binaria eclipsante y variable rs canum venaticorum de magnitud 4,21.
at magnitude 4.95. the dimmest of the seven stars of the little dipper is eta ursae minoris.

am canum venaticorum (wd 1232+37) es la estrella prototípica de esta clase de variables.
an am cvn star, or am canum venaticorum star, is a type of cataclysmic variable star.

asimismo, nashira está considerada una estrella variable alfa2 canum venaticorum con pequeñas variaciones en su brillo de 0,03 magnitudes.
it is classified as an alpha2 canum venaticorum type variable star and its brightness varies by 0.03 magnitudes.

el mecanismo podría ser similar al causante de la actividad de las estrellas variables rs canum venaticorum, o a la interacción existente entre júpiter y su luna Ío.
the mechanism may be similar to that responsible for the activity of rs canum venaticorum variable stars, or the interaction between jupiter and its moon io.

esta galaxia enana pertenece al grupo de galaxias de canes venaticorum y se halla a una distancia aproximada de 4 mpc (12 millones de años luz).
this dwarf galaxy is a member of the canes venatici group of galaxies and has a distance of about 4 mpc (12 million lightyears).

la superba (y canum venaticorum / y cvn) es una estrella de la constelación de canes venatici, notable por su profundo color rojo.
la superba (y cvn, y canum venaticorum) is a star in the constellation canes venatici, well known for its strikingly red appearance.

53 camelopardalis es una variable alfa2 canum venaticorum cuyo brillo oscila entre magnitud +5,95 y +6,08 en un ciclo de 8,2078 días.
it is classified as an alpha2 canum venaticorum type variable star and its brightness varies from magnitude +5.95 to +6.08 with a period of 8.03 days.

catalogada como variable alfa2 canum venaticorum, su brillo oscila entre magnitud aparente +6,06 y +6,09 a lo largo de un período de 2,181 días.
it is classified as an alpha2 canum venaticorum type variable star and its brightness varies from magnitude +6.06 to +6.09 with a period of 2.18 days.

== referencias ==== see also ==* hind's crimson star, r leporis - an example of a carbon star* irc +10216, cw leonis - the most studied carbon star, and also the brightest star in the sky at n-band* la superba, y canum venaticorum - one of the more bright carbon stars* marc aaronson - an american astronomer and noted researcher of carbon stars== enlaces externos ==* mcclure's paper on the carbon and related stars== referencias ==
== see also ==*barium stars*s-type stars*technetium stars*marc aaronson: an american astronomer and noted researcher of carbon starsspecimens:*r leporis, hind's crimson star: an example of a carbon star*irc +10216, cw leonis: the most studied carbon star, and also the brightest star in the sky at n-band*la superba, y canum venaticorum: one of the brighter carbon stars== references ==== external links ==*list of 110 carbon stars.