An outburst of gamma rays with energies E gamma 10 to the 12th power eV was recently detected from the X-ray pulsar Hercules X-1. The outburst had a 3 minute duration and occurred at a time during the 35 day X-ray modulation that is associated with X-ray turnon. The gamma rays also have the same 1.24 second modulation that is observed at X-ray energies. Subsequently a 40 minute outburst was detected at E gamma 10 to the 14th power eV. The interaction of ultrahigh energy particles with a precessing accretion disk explain the observed gamma ray light curve. The constraints one can place on acceleration mechanisms and the possibility that the UHE particles are accelerated by shocks in an accretion flow are explained
The cosmological gamma-ray burst (GRB) model for the production of ultra- high energy cosmic rays is...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Solar flares studied in the gamma ray region provide essential information on accelerated nuclei tha...
A signal (chance probability = .0002) with the 1.24 s period of Hercules X-1 has been observed using...
The 1.24 second binary pulsar Her X-1, first observed in X-rays in 1971 by UHURU has now been seen a...
A signal (chance probability = 2 x 10-4) with a 1.24 s period has been observed from the direction o...
High-energy gamma rays are a valuable tool for studying particle acceleration and radiation in the m...
The recently observed primary ultra high energy gamma-rays (UHEGR) testify to the cosmic ray (CR) ac...
Data from the University of Adelaide air shower array at Buckland Park taken over a three year perio...
We present RXTE monitoring of the eclipsing X-ray binary Hercules X-1 conducted over the short-high ...
We observed a large increase in the trigger rate in the direction of Hercules X-1 in the Atmospheric...
It is now more than 20 years since the first ground based gamma ray experiments involving atmospheri...
The UV emission lines of Hercules X-1, resolved with the HST GHRS and STIS, can be divided into broa...
The EGRET results for gamma ray intensities in and near the Galactic Plane have been analysed in som...
The long-standing problem of discovering the origins of ultra-high energy (UHE: E $\geq$ 10$\sp{14}$...
The cosmological gamma-ray burst (GRB) model for the production of ultra- high energy cosmic rays is...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Solar flares studied in the gamma ray region provide essential information on accelerated nuclei tha...
A signal (chance probability = .0002) with the 1.24 s period of Hercules X-1 has been observed using...
The 1.24 second binary pulsar Her X-1, first observed in X-rays in 1971 by UHURU has now been seen a...
A signal (chance probability = 2 x 10-4) with a 1.24 s period has been observed from the direction o...
High-energy gamma rays are a valuable tool for studying particle acceleration and radiation in the m...
The recently observed primary ultra high energy gamma-rays (UHEGR) testify to the cosmic ray (CR) ac...
Data from the University of Adelaide air shower array at Buckland Park taken over a three year perio...
We present RXTE monitoring of the eclipsing X-ray binary Hercules X-1 conducted over the short-high ...
We observed a large increase in the trigger rate in the direction of Hercules X-1 in the Atmospheric...
It is now more than 20 years since the first ground based gamma ray experiments involving atmospheri...
The UV emission lines of Hercules X-1, resolved with the HST GHRS and STIS, can be divided into broa...
The EGRET results for gamma ray intensities in and near the Galactic Plane have been analysed in som...
The long-standing problem of discovering the origins of ultra-high energy (UHE: E $\geq$ 10$\sp{14}$...
The cosmological gamma-ray burst (GRB) model for the production of ultra- high energy cosmic rays is...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Solar flares studied in the gamma ray region provide essential information on accelerated nuclei tha...