V1059 Sagittarii (also called Nova Sagittarii 1898) was a nova, which lit up in 1898 in the constellation Sagittarius. The star reached apparent magnitude 4.5, making it easily visible to the naked eye. It was discovered on 8 March 1898, by Williamina Fleming on a photographic plate taken at the Harvard College Observatory. The discovery plate was an objective prism plate, part of the Henry Draper Memorial Photographs, and Ms Fleming identified it as a nova based on its spectral characteristics.
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| - V1059 Sagittarii (de)
- V1059 Sagittarii (es)
- V1059 Sagittarii (fr)
- いて座V1059星 (ja)
- V1059 Sagittarii (en)
- V1059 Sagittarii (sv)
- IC 4816 (uk)
- 人马座V1059 (zh)
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| - V1059 Sagittarii es una nova avistada por los astrónomos en 1898 en la constelación de Sagitario. V1959 Sagittarii alcanzó un brillo de magnitud 4.5 . (es)
- V1059 Sagittarii war eine Nova, die 1898 im Sternbild Schütze aufleuchtete und eine Helligkeit von 4,5 mag erreichte. Der Namensteil „V1059“ folgt den Regeln zur Benennung veränderlicher Sterne und besagt, dass V1059 Sagittarii der 1059te veränderliche Stern ist, der im Sternbild Schütze (lateinisch Sagittarius) entdeckt wurde. (de)
- V1059 Sagittarii (ou Nova Sagittarii 1898) était une nova qui survint en 1898 dans la constellation du Sagittaire. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 4,5. (fr)
- いて座V1059星（V1059 Sagittarii、V1059 Sgr）は、1898年にいて座に現れた新星である。 (ja)
- V1059 Sagittarii eller Nova Sagittarii 1898 var en nova i stjärnbilden Skytten. Den upptäcktes den 18 mars 1898 av Mrs W. Fleming som under 1890-talet upptäckte ett flertal novor. Som ljusstarkast blev novan magnitud +4,5. (sv)
- IC 4816 — галактика типу S (спіральна галактика) у сузір'ї Стрілець. Цей об'єкт міститься в оригінальній редакції індексного каталогу. (uk)
- 人马座V1059（V1059 Sagittarii）是一颗位于人马座的新星，1898年爆发。 爆发后最亮视星等为4.5。 (zh)
- V1059 Sagittarii (also called Nova Sagittarii 1898) was a nova, which lit up in 1898 in the constellation Sagittarius. The star reached apparent magnitude 4.5, making it easily visible to the naked eye. It was discovered on 8 March 1898, by Williamina Fleming on a photographic plate taken at the Harvard College Observatory. The discovery plate was an objective prism plate, part of the Henry Draper Memorial Photographs, and Ms Fleming identified it as a nova based on its spectral characteristics. (en)
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| - Nova Sagittarii 1898 (en)
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| - V1059 Sagittarii es una nova avistada por los astrónomos en 1898 en la constelación de Sagitario. V1959 Sagittarii alcanzó un brillo de magnitud 4.5 . (es)
- V1059 Sagittarii war eine Nova, die 1898 im Sternbild Schütze aufleuchtete und eine Helligkeit von 4,5 mag erreichte. Der Namensteil „V1059“ folgt den Regeln zur Benennung veränderlicher Sterne und besagt, dass V1059 Sagittarii der 1059te veränderliche Stern ist, der im Sternbild Schütze (lateinisch Sagittarius) entdeckt wurde. (de)
- V1059 Sagittarii (ou Nova Sagittarii 1898) était une nova qui survint en 1898 dans la constellation du Sagittaire. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 4,5. (fr)
- V1059 Sagittarii (also called Nova Sagittarii 1898) was a nova, which lit up in 1898 in the constellation Sagittarius. The star reached apparent magnitude 4.5, making it easily visible to the naked eye. It was discovered on 8 March 1898, by Williamina Fleming on a photographic plate taken at the Harvard College Observatory. The discovery plate was an objective prism plate, part of the Henry Draper Memorial Photographs, and Ms Fleming identified it as a nova based on its spectral characteristics. The astronomical literature contains a variety of values for V1059 Sagittarii's peak brightness. Özdönmez et al. list the peak magnitude as 2.0 (visual), while Downes et al. report a much fainter value of magnitude 4.9 (photographic). Novae are usually classified as "fast" or "slow" based on the time it takes the star to drop from peak brightness by more than 3 magnitudes (T3), but for this nova the decline from maximum was poorly observed, and no T3 value has been reported. Nonetheless, it is classified as a fast nova. Vogt et al. monitored the quiescent nova 116 years after the nova event, and saw minor (0.5 to 0.8 magnitude) variations occurring at irregular intervals, similar to low amplitude dwarf nova outbursts. All novae are binary stars, with a "donor" star orbiting a white dwarf. The two stars are so close to each other that matter is transferred from the donor to the white dwarf. In the case of V1059 Sagittarii, pair's orbital period is 6.866±0.017 hours. (en)
- いて座V1059星（V1059 Sagittarii、V1059 Sgr）は、1898年にいて座に現れた新星である。 (ja)
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