标题： 新的软伽马暴源SGR1627-41的精确星际网络定位 显示英文标题

标题： Precise Interplanetary Network Localization of a New Soft Gamma Repeater, SGR1627-41

摘要： 我们介绍了乌利塞斯、KONUS-WIND和BATSE对一个在1998年6月和7月活跃的新软伽马重复暴的观测。 爆发的三角定位结果是一个约1.8度乘以16角秒的误差箱，其面积约为7.6平方角分，包含银河系超新星遗迹G337.0-0.1。 这个误差箱与BeppoSAXX射线源的位置相交，该位置也与G337.0-0.1的位置一致（Woods等，1999年），并被认为是该重复暴的平静对应体。 如果是这样的话，得到的误差箱约为2角分乘以16角秒，面积约为0.6平方角分。 误差箱在超新星遗迹中的位置表明中子星具有横向速度约为200至2000公里/秒。 显示英文摘要

摘要： We present Ulysses, KONUS-WIND, and BATSE observations of bursts from a new soft gamma repeater which was active in 1998 June and July. Triangulation of the bursts results in a ~ 1.8 degree by 16 '' error box whose area is ~ 7.6 arcminutes^2, which contains the Galactic supernova remnant G337.0-0.1. This error box intersects the position of a BeppoSAX X-ray source which is also consistent with the position of G337.0-0.1 (Woods et al. 1999), and is thought to be the quiescent counterpart to the repeater. If so, the resulting error box is ~ 2 ' by 16 '' and has an area of ~ 0.6 arcminutes^2. The error box location within the supernova remnant suggests that the neutron star has a transverse velocity of ~ 200 - 2000 km/s.