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4U 1700-37 is one of the stronger binary X-ray sources in the sky, and is classified as a high-mass X-ray binary. It was discovered by the Uhuru satellite. The "4U" designation refers to the fourth (and final) Uhuru catalog. Evidence of Compton cooling during an X-ray flare recorded by the Chandra X-ray telescope strongly suggests that the compact object is a neutron star; if verified it would be among the most massive known, and near the boundary of the theoretical maximum.

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  • 4U 1700-37 (en)
  • 4U 1700-37 (uk)
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  • 4U 1700-37 (V884 Sco) — одна з найяскравіших рентгенівських подвійних зірок на небі.Вона була відкрита супутником Ухуру.Позначення «4U» означає четвертий (і останній) каталог Ухуру. До системи входить яскравий (6.53 V зоряної величини) надгігант класу Of HD 153919 і компактний об'єкт з акреційним диском, який може бути нейтронною зорею або чорною дірою.Кожні 3,4 доби відбувається затемнення рентгенівського джерела зорею. Рентгенівські пульсації у системі не спостерігалися. Джерело є одним з 10 найяскравіших на небі постійних джерел у жорсткому рентгенівському діапазоні 10-100 кеВ. (uk)
  • 4U 1700-37 is one of the stronger binary X-ray sources in the sky, and is classified as a high-mass X-ray binary. It was discovered by the Uhuru satellite. The "4U" designation refers to the fourth (and final) Uhuru catalog. Evidence of Compton cooling during an X-ray flare recorded by the Chandra X-ray telescope strongly suggests that the compact object is a neutron star; if verified it would be among the most massive known, and near the boundary of the theoretical maximum. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V884ScoLightCurve.png
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  • −6.52 (en)
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  • +0.253 (en)
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  • O6Iafcp (en)
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  • O star (en)
  • X-ray object (en)
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