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Spin evolution of NSs

Spin evolution of NSs

Spin evolution of NSs. Evolution of neutron stars. Magneto- rotational. Thermal. Observational appearence of a NS can depend on: Temperature Period Magnetic field Velocity. Evolution of NSs: temperature. Neutrino cooling stage. Photon cooling stage. First papers on the thermal

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437 views • 43 slides
Spin evolution of NSs

Spin evolution of NSs

Spin evolution of NSs. Evolution of neutron stars. Magneto- rotational. Thermal. Observational appearence of a NS can depend on: Temperature Period Magnetic field Velocity. Evolution of NSs: temperature. Neutrino cooling stage. Photon cooling stage. First papers on the thermal

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404 views • 40 slides
David Fushman Department of Chemistry & Biochemistry University of Maryland, College Park

David Fushman Department of Chemistry & Biochemistry University of Maryland, College Park

Virtual NMR Spectrometer a software package for accurate and efficient calculation of the outcome of NMR experiments and a computer tool for learning NMR . David Fushman Department of Chemistry & Biochemistry University of Maryland, College Park. 90 o. 90 o. t1. d1.

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1.26k views • 29 slides
Monte-Carlo experiments on NS Spin Evolution of BeXBs

Monte-Carlo experiments on NS Spin Evolution of BeXBs

Monte-Carlo experiments on NS Spin Evolution of BeXBs. arXiv:1111.2051v1 (Christian Knigge,etal) arXiv:1101.5036v1 (Pablo Reig)

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325 views • 23 slides
The Cosmic Density and Distribution of Relativistic Iron Lines

The Cosmic Density and Distribution of Relativistic Iron Lines

The Cosmic Density and Distribution of Relativistic Iron Lines. David R. Ballantyne Center for Relativistic Astrophysics, School of Physics, Georgia Tech. 2010, ApJ, 708, L1. Motivation. Relativistic Fe K ? lines are v. important for probing the physics of the inner accretion flow

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239 views • 14 slides
Spin and Orbital Evolution of the Accreting Millisecond Pulsar SAX J1808.4-3658:

Spin and Orbital Evolution of the Accreting Millisecond Pulsar SAX J1808.4-3658:

Spin and Orbital Evolution of the Accreting Millisecond Pulsar SAX J1808.4-3658: Implications for Gravitational Wave Searches. Deepto Chakrabarty Massachusetts Institute of Technology. Featuring Ph.D. thesis work of Jacob M. Hartman at MIT.

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305 views • 14 slides

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