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ИСТИНА ЦЭМИ РАН |
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This is specific meeting devoted to fascinating stellar explosions, including all recent advances from both the theoretical and the observational points of view. The aim of this conference was to focter contacts within the different experts in the field, including observers and theoreticians, in order to address the current knowledge, outstanding problems and future perspectives in the field of classical novae. The programme of the conference consisted of 8 sessions: scenario, explosion mechanism and mass loss; observations in optical,UV,IR and radio spectra; model atmospheres and light curves; X-rays from novae; gamma-rays from novae; nova population/novae in external galaxies; old nova shells and remnants.