High Energy Emission from Four New Radio Pulsars

Details High Energy Emission from Four New Radio Pulsars High Energy Emission from Four New Radio Pulsars

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.9304z&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #93.04; Bulletin of the American Astronomical Society, Vol. 25, p.1435

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Scientific paper

In a independent survey of compact sources in the Einstein IPC data, we obtained X-ray targets used in a search for radio pulsars at the Arecibo Observatory. About 1500 such targets have been observed, resulting in the discovery of three new radio pulsars: PSR J0631+10, J1843+20 and J1908+04. The first one is a young pulsar (age ~ 43000 years) with a flat radio spectrum that hints to strong scattering near 430 MHz. The last one is in the same radio beam as a know pulsar, B1905+04, suggesting that many pulsars may have gone undetected in previous radio surveys. In another project, we discovered a 3.5 millisecond pulsar inside a EGRET gamma-ray error box. We present here the latest results in the search for association between pulsar and high energy source.

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