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- BH dels Llebrers (BH Canum Venaticorum) és un estel variable en la constel·lació dels Llebrers, els gossos de caça. La seva magnitud aparent mitjana és +4,93 —la vuitena més brillant en la seva constel·lació— i es troba a 145 anys llum del sistema solar. (ca)
- HR 5110, also known as BH Canum Venaticorum, is a binary star system in the northern constellation of Canes Venatici. It is visible to the naked eye with an apparent visual magnitude of 4.91. Based upon an annual parallax shift of 21.90±0.23 mas, it is located 149 light-years away. The system is moving further from the Sun with a heliocentric radial velocity of 6.4 km/s. This is a close binary system with an orbital period of 2.6 days and an orbital plane that is oriented nearly face-on. It may be considered an Algol-type semidetached binary. The hotter primary component has a stellar classification of F2 IV, indicating it is an evolving subgiant star that is leaving the main sequence after consuming the hydrogen at its core. HR 5110 is classified as a RS Canum Venaticorum variable system, primarily due to chromospheric activity in the secondary component. This star has a classification of K0 IV, matching a K-type subgiant star. Based upon the close separation of the pair and the class of the secondary component, that latter is probably filling its roche lobe. This star is most likely the source of the radio emission from this system, and the alignment of this signal is consistent with a polar starspot. (en)
- BH Canum Venaticorum (BH CVn) es una estrella variable en la constelación de Canes Venatici, los perros de caza.Su magnitud aparente media es +4,93 —la octava más brillante en su constelación— y se encuentra a 145 años luz del Sistema Solar. (es)
- 南十字座BH，又名BD+37 2426，HD 118216、SAO 63623、HR 5110，是南十字座的一颗恒星，视星等为4.98，位于銀經83.33，銀緯76.41，其B1900.0坐标为赤經13h 30m 19.9s，赤緯+37° 76.41′ 41″。 (zh)
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- BH dels Llebrers (BH Canum Venaticorum) és un estel variable en la constel·lació dels Llebrers, els gossos de caça. La seva magnitud aparent mitjana és +4,93 —la vuitena més brillant en la seva constel·lació— i es troba a 145 anys llum del sistema solar. (ca)
- BH Canum Venaticorum (BH CVn) es una estrella variable en la constelación de Canes Venatici, los perros de caza.Su magnitud aparente media es +4,93 —la octava más brillante en su constelación— y se encuentra a 145 años luz del Sistema Solar. (es)
- 南十字座BH，又名BD+37 2426，HD 118216、SAO 63623、HR 5110，是南十字座的一颗恒星，视星等为4.98，位于銀經83.33，銀緯76.41，其B1900.0坐标为赤經13h 30m 19.9s，赤緯+37° 76.41′ 41″。 (zh)
- HR 5110, also known as BH Canum Venaticorum, is a binary star system in the northern constellation of Canes Venatici. It is visible to the naked eye with an apparent visual magnitude of 4.91. Based upon an annual parallax shift of 21.90±0.23 mas, it is located 149 light-years away. The system is moving further from the Sun with a heliocentric radial velocity of 6.4 km/s. (en)
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- BH dels Llebrers (ca)
- BH Canum Venaticorum (es)
- HR 5110 (en)
- BH Canum Venaticorum (sv)
- 南十字座BH (zh)
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