Associating Young Pulsars and Supernova Remnants: PSR 1610-50 and the Case for High-Velocity Pulsars
Associating Young Pulsars and Supernova Remnants: PSR 1610-50 and the Case for High-Velocity Pulsars
复制标题
将年轻脉冲星和超新星遗迹联系起来：PSR 1610-50 和高速脉冲星的案例
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发表时间：
1993
期刊：
影响因子：
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通讯作者：
P. Caraveo
中科院分区：
文献类型：
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作者：
P. Caraveo
在1990年代，卫星和信噪比之间的联系数量急剧增加，从1988年的5个增加到1993年初的11个。这部分是由于新的脉冲星调查，部分是由于临时搜索，部分是由于脉冲星和信噪比目录之间的后验互相关。从表面上看，所有提出的鉴定，人们发现，在最新的目录中列出的10个最年轻的恒星中，有9个与SNR有关（泰勒，曼彻斯特和莱恩1993）。PSR 1610-50是个例外，它是第四年轻的脉冲星，是最近在一次脉冲星巡天中发现的（约翰斯顿等，1992）。在这里，我们提出的协会，这7500岁的脉冲星与Kes 32，一个著名的信噪比可比的年龄和距离
The number of associations between pulsars and SNRs has grown dramatically in the 1990s, going from a total of five in 1988 to 11 at the beginning of 1993. This is due in part to new pulsar surveys, in part to ad hoc searches and in part to a posteriori cross-correlations between pulsar and SNR catalogs. Taking at face value all the proposed identifications, one finds that nine of the 10 youngest pulsars, listed in the most recent catalog (Taylor, Manchester, & Lyne 1993), are associated with a SNR. The exception is PSR 1610-50, the fourth youngest pulsar, recently discovered during a pulsar survey (Johnston et al. 1992). Here we propose the association of this 7500 yr old pulsar with Kes 32, a well-known SNR of comparable age and distance