CT Serpentis (also known as Nova Serpentis 1948) was a nova that appeared in the constellation Serpens in 1948. It was discovered by Ramze Alexander Bartaya at Abastumani Observatory on 9 April 1946. It is thought to have reached magnitude 6.0, but this is an extrapolation of its light curve as it was not observed until 9 April 1948 when it was at magnitude 9.0 and fading—clearly past its maximum.
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| - CT Serpentis (de)
- CT Serpentis (en)
- CT Serpentis (sv)
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| - CT Serpentis (auch Nova Serpentis 1948) war eine Nova, die im Jahr 1948 im Sternbild Schlange erschien und mit dem 30. September 1948 verzeichnet wurde. Es wird angenommen, dass sie eine Helligkeit von mindestens 6,0 mag erreichte, wobei dies eine Extrapolation ihrer Lichtkurve war. Die Nova erreichte eine tatsächliche Helligkeit von 9,0m und verblasste anschließend. (de)
- CT Serpentis (also known as Nova Serpentis 1948) was a nova that appeared in the constellation Serpens in 1948. It was discovered by Ramze Alexander Bartaya at Abastumani Observatory on 9 April 1946. It is thought to have reached magnitude 6.0, but this is an extrapolation of its light curve as it was not observed until 9 April 1948 when it was at magnitude 9.0 and fading—clearly past its maximum. (en)
- CT Serpentis eller Nova Serpentis 1948 var en snabb nova i stjärnbilden Ormen. Novan upptäcktes den 18 februari 1948 av den georgiske astronomen R. Bartaya. Den nådde magnitud +6,0 i maximum och avklingade sedan snabbt. Den är nu en stjärna av 16:e magnituden. (sv)
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| - CT Serpentis (auch Nova Serpentis 1948) war eine Nova, die im Jahr 1948 im Sternbild Schlange erschien und mit dem 30. September 1948 verzeichnet wurde. Es wird angenommen, dass sie eine Helligkeit von mindestens 6,0 mag erreichte, wobei dies eine Extrapolation ihrer Lichtkurve war. Die Nova erreichte eine tatsächliche Helligkeit von 9,0m und verblasste anschließend. (de)
- CT Serpentis (also known as Nova Serpentis 1948) was a nova that appeared in the constellation Serpens in 1948. It was discovered by Ramze Alexander Bartaya at Abastumani Observatory on 9 April 1946. It is thought to have reached magnitude 6.0, but this is an extrapolation of its light curve as it was not observed until 9 April 1948 when it was at magnitude 9.0 and fading—clearly past its maximum. (en)
- CT Serpentis eller Nova Serpentis 1948 var en snabb nova i stjärnbilden Ormen. Novan upptäcktes den 18 februari 1948 av den georgiske astronomen R. Bartaya. Den nådde magnitud +6,0 i maximum och avklingade sedan snabbt. Den är nu en stjärna av 16:e magnituden. (sv)
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