The "Black Widow" Pulsar PSR 1957+20: A Potential VHE [gamma]-ray Source |
Contents
The Eclipsing Millisecond Binary Pulsar PSR 1957+20 | 10 |
The HGO Telescope | 45 |
5 | 51 |
2 other sections not shown
Common terms and phrases
accept air showers analysis aperture assumed average background binary calculated channel Chapter companion consistent corresponding cosmic ray counting rate data set delays density derivative described detection determined direction discussed displayed displayed in Figure distribution duration eclipse effect emission energy entire ergs event excess expected Figure flux frequency function given hadronic HGO telescope hypothesis indicate initiated integrated light curve limit luminosity magnetic field mass matter mean measured mirror multiplicity neutron star night sky nsec coincidence width observed optical orbital orbital phase parameters period phase photoelectron Physics polar position possible presence primary probability pulsar pulse radio radius region reject reported represents requires respect result secondary showed signal significance single source data spectrum statistic stellar wind Table threshold typical unit University wind y-ray zenith angle