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- EU Andromedae (often abbreviated to EU And) is a carbon star in the constellation Andromeda. Its apparent visual magnitude varies in an irregular manner between 10.7 and 11.8. Infrared observations of EU Andromedae show the presence of silicate grains, indicating the presence of an oxygen-rich circumstellar shell around the star, a combination known as a silicate star. Subsequently, a water maser was detected around this star (and for the first time around a carbon star), confirming the existence of the shell. The most recent observations suggest that the maser originated in a circumstellar disc, seen nearly edge-on, around an unseen companion with a minimum mass of 0.5 M☉. Carbon dioxide has been detected for the first time in a silicate carbon star around EU Andromedae. EU Andromedae is given as the standard star for the C-J5− spectral class. C-J spectral types are assigned to stars with strong isotopic bands of carbon molecules, defined as the ratio of 12C to 13C being less than four. A more complete spectral type includes the abundance indices C25 j3.5, which indicate the Swan band strength and the isotopic band ratio. (en)
- EU Андромеды (лат. EU Andromedae) — одиночная переменная звезда в созвездии Андромеды на расстоянии приблизительно 5006 световых лет (около 1535 парсеков) от Солнца. Видимая звёздная величина звезды — от +11,8m до +10,7m. (ru)
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- 4.018000 (xsd:double)
- 4.492000 (xsd:double)
- 5.526000 (xsd:double)
- 9.000500 (xsd:double)
- 10.380000 (xsd:double)
- 12.840000 (xsd:double)
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- EU Андромеды (лат. EU Andromedae) — одиночная переменная звезда в созвездии Андромеды на расстоянии приблизительно 5006 световых лет (около 1535 парсеков) от Солнца. Видимая звёздная величина звезды — от +11,8m до +10,7m. (ru)
- EU Andromedae (often abbreviated to EU And) is a carbon star in the constellation Andromeda. Its apparent visual magnitude varies in an irregular manner between 10.7 and 11.8. Infrared observations of EU Andromedae show the presence of silicate grains, indicating the presence of an oxygen-rich circumstellar shell around the star, a combination known as a silicate star. Subsequently, a water maser was detected around this star (and for the first time around a carbon star), confirming the existence of the shell. The most recent observations suggest that the maser originated in a circumstellar disc, seen nearly edge-on, around an unseen companion with a minimum mass of 0.5 M☉. Carbon dioxide has been detected for the first time in a silicate carbon star around EU Andromedae. (en)
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- EU Andromedae (en)
- EU Андромеды (ru)
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