ASCA studies of young pulsars and SNRs

被引：0
|
作者：
Torii, K
Kinugasa, K
Asanuma, T
Toneri, T
Tsunemi, H
Dotani, T
Mitsuda, K
Gotthelf, EV
Petre, R
机构：
[1] Natl Space Dev Agcy Japan, Space Utilizat Res Program, Tsukuba Space Ctr, Tsukuba, Ibaraki 3058505, Japan
[2] Gunma Astron Observ, Maebashi, Gumma 3710847, Japan
[3] Osaka Univ, Dept Earth & Space Sci, Grad Sch Sci, Toyonaka, Osaka 5600043, Japan
[4] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[5] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA
来源：
BROAD BAND X-RAY SPECTRA OF COSMIC SOURCES | 2000年 / 25卷 / 3-4期
关键词：
D O I：
10.1016/S0273-1177(99)00819-4
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
During the course of our X-ray studies of composite supernova remnants, we have discovered two young pulsars, The 65 ms pulsar, AX J1811.5-1926, is found to be associated with the central X-ray emission from the candidate of the historical SNR G11.2-0.3; and the 69 ms pulsar near the SNR RCW 103 is identified with a previously reported GINGA pulsator. Here, we present an observational summary of these two pulsars. (C) 2000 COSPAR. Published by Elsevier Science Ltd.
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收藏
页码：669 / 672
页数：4
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