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RS Canum Venaticorum variable: 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 large stellar spots. (Astronomy) [100%] 2023-09-08 [RS Canum Venaticorum variables] [Binary stars]...
Alpha2 Canum Venaticorum variable: An Alpha Canum Venaticorum variable (or α CVn variable) is a type of variable star. These stars are chemically peculiar main sequence stars of spectral class B8p to A7p. (Astronomy) [100%] 2022-10-09 [Alpha2 Canum Venaticorum variables]
Alpha2 Canum Venaticorum variable: An Alpha Canum Venaticorum variable (or α CVn variable) is a type of variable star. These stars are chemically peculiar main sequence stars of spectral class B8p to A7p. (Variable star type) [100%] 2024-10-14 [Alpha2 Canum Venaticorum variables]
Alfa Canum Venaticorum: Se encuentra a 110 años luz del sistema solar. Nombre[editar] El nombre Cor Caroli («Corazón de Carlos») fue asignado en 1725 por el astrónomo Edmund Halley en honor del rey Carlos II de Inglaterra, a sugerencia del físico de ... [83%] 2023-05-17
24 Canum Venaticorum: Con magnitud aparente +4,70, es la tercera estrella más brillante de la constelación después de Cor Caroli (α Canum Venaticorum) y Asterion (β Canum Venaticorum). Situada a 191 años luz del sistema solar, 24 Canum Venaticorum es una estrella blanca de ... [83%] 2023-05-17
6 Canum Venaticorum: 6 Canum Venaticorum is a single star in the northern constellation Canes Venatici, located 246 light years from the Sun. It is visible to the naked eye as a faint yellow-hued star with an apparent visual magnitude of +5 ... (Astronomy) [83%] 2023-07-15 [G-type giants] [Horizontal-branch stars]...
20 Canum Venaticorum: Aun teniendo magnitud aparente +4,72 no tiene denominación de Bayer. A 286 años luz de distancia del sistema solar, AO Canum Venaticorum es una gigante blanco-amarilla de tipo espectral F3III. Con una temperatura efectiva de 7046 K, es ... [83%] 2023-05-17
Beta Canum Venaticorum: De magnitud aparente +4,26, es la segunda estrella más brillante de la constelación después de Cor Caroli (α Canum Venaticorum). Distante 27,4 años luz del sistema solar, las estrellas conocidas más próximas a Asterion son Gliese 450 y Groombridge ... [83%] 2023-06-01
R Canum Venaticorum: R Canum Venaticorum is a Mira variable star in the constellation Canes Venatici. It ranges between magnitudes 6.5 and 12.9 over a period of approximately 329 days. (Astronomy) [83%] 2024-01-26 [Mira variables] [Canes Venatici]...
4 Canum Venaticorum: 4 Canum Venaticorum is a binary star system in the northern constellation of Canes Venatici, located around 425 light years away. It has the variable star designation AI Canum Venaticorum; 4 Canum Venaticorum is its Flamsteed designation. (Astronomy) [83%] 2024-01-26 [F-type subgiants] [F-type giants]...
6 Canum Venaticorum: 6 Canum Venaticorum (6 CVn) es una estrella en la constelación de Canes Venatici, los lebreles. Tiene magnitud aparente +5,02 —la décima más brillante en su constelación— y se encuentra, de acuerdo a la nueva reducción de datos de ... [83%] 2024-01-19
6 Canum Venaticorum: 6 Canum Venaticorum is a single star in the northern constellation Canes Venatici, located 246 light years from the Sun. It is visible to the naked eye as a faint yellow-hued star with an apparent visual magnitude of +5 ... (Star in the constellation Canes Venatici) [83%] 2023-08-18 [G-type giants] [Horizontal-branch stars]...
8 Canum Venaticorum: De magnitud aparente +4,26, es la segunda estrella más brillante de la constelación después de Cor Caroli (α Canum Venaticorum). Distante 27,4 años luz del sistema solar, las estrellas conocidas más próximas a Asterion son Gliese 450 y Groombridge ... [83%] 2023-05-17
DG Canum Venaticorum: 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 of 0.20″ along a position angle of 285°, which corresponds to a physical separation ... (Astronomy) [83%] 2023-10-22 [Canes Venatici] [M-type main-sequence stars]...
10 Canum Venaticorum: 10 Canum Venaticorum is the Flamsteed designation for an ordinary star in the northern constellation of Canes Venatici. It has an apparent visual magnitude of 5.95, which, according to the Bortle scale, can be faintly seen with the naked ... (Astronomy) [83%] 2023-07-09 [Canes Venatici] [G-type main-sequence stars]...
21 Canum Venaticorum: BK Canum Venaticorum Datos de observación (Época J2000. Tiene magnitud aparente +5,15 y está situada a 275 años luz del sistema solar. BK Canum Venaticorum es una estrella blanca de la secuencia principal de tipo espectral A0V, el mismo que ... [83%] 2023-05-17
AM Canum Venaticorum: AM Canum Venaticorum (AM CVn) is a hydrogen-deficient cataclysmic variable binary star in the constellation of Canes Venatici. It is the type star of its class of variables, the AM Canum Venaticorum stars. (Astronomy) [83%] 2024-01-07 [Canes Venatici] [AM CVn stars]...
AW Canum Venaticorum: AW Canum Venaticorum is a variable star in the constellation Canes Venatici. It is visible to the naked eye with a nominal apparent visual magnitude of 4.76. (Astronomy) [83%] 2023-12-04 [M-type giants] [Semiregular variable stars]...
RS Canum Venaticorum: RS Canum 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. (Astronomy) [83%] 2023-11-23 [F-type main-sequence stars] [K-type subgiants]...
5 Canum Venaticorum: 5 Canum Venaticorum is a probable binary star system in the northern constellation of Canes Venatici, located about 375 light years from the Sun. It is visible to the naked eye as a faint, yellow-hued star with an apparent ... (Probable binary star system in the constellation Canes Venatici) [83%] 2022-11-13 [G-type giants] [Barium stars]...