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《ACTA ASTRONOMICA SINICA》 1994-01
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THE IDENTIFICATION OF THE NEW γ-RAY PULSAR PSR1055-52 FROM COS-B DATA

Song Li-ming; Lu Tan (Astronomy Department of Nanjing University, Nanjing 210008)  
Using the COS-B data, we analysed the timing parameters of the γ-ray pulsar PSR1055-52 newly discovered by Compton GRO and found the significant pulsed phase structure quite similar to that found by CGRO. This result provides an independent support for the PSR1055-52 to be a γ-ray pulsar. This γ-ray pulsar is also compared with other 5 widely known ones.
【Fund】: 国家攀登计划和教委博士点基金
【CateGory Index】: P145.6
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