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- GP Comae Berenices, abbreviated to GP Com and also known as G 61-29, is a star system composed of a white dwarf orbited by a planetary mass object, likely the highly eroded core of another white dwarf star. The white dwarf is slowly accreting material from its satellite at a rate of (3.5±0.5)×10−11 M☉/year and was proven to be a low-activity AM CVn star. The star system is showing signs of a high abundance of ionized nitrogen from the accretion disk around the primary. (en)
- GP Волос Вероники (лат. GP Comae Berenices) — двойная катаклизмическая переменная звезда типа AM Гончих Псов (AM)* в созвездии Волосы Вероники на расстоянии приблизительно 238 световых лет (около 72,8 парсека) от Солнца. Видимая звёздная величина звезды — от +16,29m до +15,69m. Орбитальный период — около 0,03234 суток (0,7761 часа). (ru)
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- GP Comae Berenices, abbreviated to GP Com and also known as G 61-29, is a star system composed of a white dwarf orbited by a planetary mass object, likely the highly eroded core of another white dwarf star. The white dwarf is slowly accreting material from its satellite at a rate of (3.5±0.5)×10−11 M☉/year and was proven to be a low-activity AM CVn star. The star system is showing signs of a high abundance of ionized nitrogen from the accretion disk around the primary. (en)
- GP Волос Вероники (лат. GP Comae Berenices) — двойная катаклизмическая переменная звезда типа AM Гончих Псов (AM)* в созвездии Волосы Вероники на расстоянии приблизительно 238 световых лет (около 72,8 парсека) от Солнца. Видимая звёздная величина звезды — от +16,29m до +15,69m. Орбитальный период — около 0,03234 суток (0,7761 часа). (ru)
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- GP Comae Berenices (en)
- GP Волос Вероники (ru)
- GP Comae Berenices (sv)
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