Very high energy gamma rays from PSR 1706-44
نویسندگان
چکیده
منابع مشابه
A pr 1 99 8 TeV gamma rays from PSR 1706 - 44
Observations made with the University of Durham Mark 6 atmospheric Čerenkov telescope confirm that PSR B1706-44 is a very high energy γ-ray emitter. There is no indication from our dataset that the very high energy γ-rays are pulsed, in contrast to the findings at < 20 GeV, which indicate that more than 80% of the flux is pulsed. The flux at E > 300 GeV is estimated to be (3.9±0.7stat)×10 −11 c...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 1995
ISSN: 0004-637X,1538-4357
DOI: 10.1086/187723