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- SGR 1627-41 est un sursauteur gamma mou situé dans la constellation de la Règle. Il s'agit d'un des trois sursauteurs gamma mous identifiés avec certitude à ce jour (2007) au sein de notre Galaxie, avec SGR 1806-20 et SGR 1900+14. Il a été découvert en 1998. (fr)
- SGR 1627−41, is a soft gamma repeater (SGR), located in the constellation of Ara. It was discovered June 15, 1998 using the Burst and transient Source Experiment (BATSE) and was the first soft gamma repeater to be discovered since 1979. During a period of 6 weeks, the star bursted approximately 100 times, and then went quiet. The measured bursts lasted an average of 100 milliseconds, but ranged from 25 ms to 1.8 seconds. SGR 1627−41 is a persistent X-ray source. It is located at a distance of 11 kpc in the radio complex CTB 33, a star forming region that includes the supernova remnant G337.0-0.1. This object is believed to be a neutron star that undergoes random outbursts of hard and soft X-rays. This may be caused by the loss of angular momentum of a highly magnetized neutron star, or magnetar. Alternatively, it may be a quark star, although this is considered less likely. After the 1998 outburst and the 40-day afterglow, SGR 1627−41 has remained dormant and is steadily cooling down from the peak during the event. (en)
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- SGR 1627-41 est un sursauteur gamma mou situé dans la constellation de la Règle. Il s'agit d'un des trois sursauteurs gamma mous identifiés avec certitude à ce jour (2007) au sein de notre Galaxie, avec SGR 1806-20 et SGR 1900+14. Il a été découvert en 1998. (fr)
- SGR 1627−41, is a soft gamma repeater (SGR), located in the constellation of Ara. It was discovered June 15, 1998 using the Burst and transient Source Experiment (BATSE) and was the first soft gamma repeater to be discovered since 1979. During a period of 6 weeks, the star bursted approximately 100 times, and then went quiet. The measured bursts lasted an average of 100 milliseconds, but ranged from 25 ms to 1.8 seconds. SGR 1627−41 is a persistent X-ray source. It is located at a distance of 11 kpc in the radio complex CTB 33, a star forming region that includes the supernova remnant G337.0-0.1. (en)
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- SGR 1627-41 (fr)
- SGR 1627−41 (en)
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