... 19:45 . End of Day 2 . 22/12 . NEUTRON STARS . 09:30 . 00:35 . J.Truemper . ... 00:35 . J.Truemper . Progress and puzzles in neutron star physics . 10:05 . 00:25 . ... of thermonuclear burning along the surface of neutron star for high-frequency ...
... Пширков М.С. Попов С.Б. A new method is suggested to search for axions constituting Dark Matter that utilizes observations of neutron stars (NS) in radio-frequency region. ...
... neutron stars with strong magnetic fields: progress and vistas Alexander Y ... neutron stars Case of CCO 1E 1207.4-5209 Atmosphere models for heavier elements K ... neutron stars Cyclotron harmonics in spectra of isolated neutron stars Accurate ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/21/Potehin.pdf -- 2793.7 Кб -- 26.01.2011 Похожие документы
... neutron star equations of state and the equation As matter accretes onto a neutron star from the accretion disk, its ... neutrons, located quite close to the surface of the neutron star, can undergo several processes, one of which is the H(n,)D ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B35_Caliskan01-05May07_00:06:06.pdf -- 207.7 Кб -- 04.05.2007 Похожие документы
... amplitudes courtesy Anna Watts 7 Theory of torsional vibrations of neutron stars: 1 ... 2000's Steiner & Watts 09 Theory of torsional vibrations of neutron stars: 3 ... 20 Hz QPO as an edge mode for normal proton fraction, decoupled neutrons 2. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/21/Levin.pdf -- 2594.3 Кб -- 26.01.2011 Похожие документы
... The line shapes thus change with free falling plasma free falling plasma shock slowly sinking plasma layer of radiation neutron star neutron star Figure 2. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G41_Schoenherr01-07Feb07_16:54:04.pdf -- 385.0 Кб -- 07.02.2007 Похожие документы
... neutron star surface are compatible with the presence of a disk around the neutron ... neutron star crust is the It was proposed some years ago that the different ... neutron star acts as a "gyrostat"- the equilibrium period is: Peq = µ 6/7 (dM/dt) -3 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I04_Alpar01-30May07_18:14:26.pdf -- 38.9 Кб -- 30.05.2007 Похожие документы
... A. Bogomazov . Mass evolution of binary neutron stars. poster C2 . V. Bogomolov . ... model of turbulence to simulations of thermonuclear bursts of neutron stars in LMXB ... Suprathermal radial pulsations of neutron stars (authors: M.E. Gusakov, D.G ...