Accretion Processes in Astrophysics: Proceedings of the Twenty-first Rencontre de Moriond, Astrophysics Meeting, Les Arcs, Savoie, France, March 9-16, 1986J. Thanh Van Tran, Jean Audouze Atlantica Séguier Frontières, 1986 - 215 lappuses |
Saturs
ELBERT J W Ultrahighenergy gamma rays observed | 1 |
SVOBODA R Recent results from the IMB detector | 17 |
WEEKES T C CygnusX3 source of very high energy | 37 |
WEEKES T C Very high energy gammaray observations | 57 |
GAISSER T K High energy neutrinos in close binary stars | 77 |
Citi izdevumi - Skatīt visu
Bieži izmantoti vārdi un frāzes
acceleration accretion rate assumed Astrophys atmosphere background binary black hole burst calculations carbon central collapse companion compared cosmic ray curve Cygnus X-3 decay deflagration density depends detected detector direction discussed disk distance distribution effects emission emitted estimate et al evidence excess expected experiments field Figure final flash flux gamma gamma-ray give given heat high energy hour ignition increase indicate initial interaction layers light limit lower luminosity mass material matter measured muon Nature neutrino neutron star Nomoto object observed obtained occur optical outburst parameter particles peak period phase Physics possible present probably produced protons pulsar radiation range reaction region reported scale seen shower shown shows signal significant solid spectra spectrum stellar surface Table taken temperature thick transients University white dwarf wind X-ray