| dbo:abstract |
R Fornacis is a Mira variable and carbon star located in the constellation Fornax. It is around 1,800 light years away based on parallax measurements. R Fornacis is a carbon star, a star on the asymptotic giant branch with an excess of carbon over oxygen in its atmosphere due to fusion products being dredged up to the surface from deep inside the star. It is also a Mira variable, a type of pulsating giant star which varies by several apparent magnitudes with a period of a few hundred days. R Fornacis has a period of 389 days and varies between extremes of magnitude 7.5 and 13.0, although average maximum and minimum magnitudes are 8.9 and 12.2 respectively.. R Fornacis was discovered to be variable in 1896 after it had been observed with a different brightness to that shown in the Cordoba Durchmusterung. In 1983, an unusually deep minimum was observed, and later correlated with an asymmetric shell of material ejected from the surface of the star. Unconfirmed visual estimates of the unusual minimum give a magnitude of 14.0, while infrared observations confirm the unusual variation. (en) R Fornacis är en pulserande variabel av Mira Ceti-typ (M) i stjärnbilden Ugnen. Stjärnan var den första i Ugnens stjärnbild som fick en variabelbeteckning. Stjärnan varierar mellan visuell magnitud +7,5 och 13,0 med en period av 386 dygn. (sv) |
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wiki-commons:Special:FilePath/RForLightCurve.png?width=300 |
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J (en) |
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C4,3e (en) |
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| dbp:parallax |
1.806900 (xsd:double) |
| dbp:propMoDec |
−3.957 (en) |
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| rdfs:comment |
R Fornacis är en pulserande variabel av Mira Ceti-typ (M) i stjärnbilden Ugnen. Stjärnan var den första i Ugnens stjärnbild som fick en variabelbeteckning. Stjärnan varierar mellan visuell magnitud +7,5 och 13,0 med en period av 386 dygn. (sv) R Fornacis is a Mira variable and carbon star located in the constellation Fornax. It is around 1,800 light years away based on parallax measurements. R Fornacis is a carbon star, a star on the asymptotic giant branch with an excess of carbon over oxygen in its atmosphere due to fusion products being dredged up to the surface from deep inside the star. It is also a Mira variable, a type of pulsating giant star which varies by several apparent magnitudes with a period of a few hundred days. R Fornacis has a period of 389 days and varies between extremes of magnitude 7.5 and 13.0, although average maximum and minimum magnitudes are 8.9 and 12.2 respectively.. (en) |
| rdfs:label |
R Fornacis (en) R Fornacis (sv) |
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