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Documents January 8, 2003201st AAS Meeting1 Nucleosynthesis, Pulsars, Cosmic Rays, and Shock Physics: High...

Slide 1 January 8, 2003201st AAS Meeting1 Nucleosynthesis, Pulsars, Cosmic Rays, and Shock Physics: High Energy Studies of Supernova Remnants with Chandra and XMM-Newton…

Documents COOLING OF N EUTRON ST A R S

COOLING OF NEUTRON STARS D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Huntsville – May – 2009 Introduction Neutrino emission Cooling theory…

Documents Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute.

Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute DCR-1000 - cross 1000х1000 m, width 40 m, range 30-120 MHz. BSA – array of 16384 dipoles,187х384 m, 16…

Documents Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute

Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute DCR-1000 - cross 1000х1000 m, width 40 m, range 30-120 MHz. BSA – array of 16384 dipoles,187х384 m, 16…

Documents Spatial/Spectral Studies of Supernova Remnants with Chandra and XMM-Newton John P. Hughes

Spatial/Spectral Studies of Supernova Remnants with Chandra and XMM-Newton John P. Hughes Rutgers University Constellation-X Workshop New Pulsars and CCOs Cas A CXOU J232327.9+584842…

Documents COOLING OF N EUTRON ST A R S

COOLING OF NEUTRON STARS D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Ladek Zdroj, February 2008, 1. Formulation of the Cooling Problem 2. Superlfuidity…

Documents COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS

COOLING NEUTRON STARS: THEORY AND OBSERVATIONS D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Hirschegg – January – 2009 Introduction Neutrino…

Documents THERMAL EVOLUTION OF N EUTRON ST A R S: Theory and observations

THERMAL EVOLUTION OF NEUTRON STARS: Theory and observations D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Catania, October 2012, 1. Formulation…