1140029
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资源简介：
PSR B1259-63 is a gamma-ray binary comprising a radio pulsar in orbit around a Be star. To study the hard X-ray activity after the next periastron passage happening within AO11 perhaps concurrent with a new GeV flare we propose a series of INTEGRAL observations with total exposure of 800 ks. These observations will provide a unique chance to understand the hard X-ray emission after periastron and shed light on the nature of the possible GeV flare. [truncated! Please see actual data for full text]
创建时间：
2025-03-14
