100+ J0737 PowerPoint (PPT) Presentations, J0737 PPTs

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Lecture1. Structure of Neutron Stars

Lecture1. Structure of Neutron Stars. Sergei Popov (SAI MSU). Artistic view . For NSs we can take T=0 and neglect the third equation. Hydrostatic equilibrium for a star. For a NS effects of GR are also important. M/R ~ 0.15 (M/M ? ) (R/10 km ) -1 J/M ~ 0.25 (1 ms/P) (M/M ? )(R/10km) 2.

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784 views • 63 slides

Neutron Star (Mostly Pulsar) Masses

Neutron Star (Mostly Pulsar) Masses. Ingrid Stairs UBC Vancouver CAWONAPS TRIUMF Dec. 9, 2010. Pulsars are one manifestation of neutron stars: spin periods ~ 1.4 ms to 8.5 seconds, magnetic fields ~10 8 to ~5 x10 13 G. Low fluxes mean large radio telescopes

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288 views • 20 slides

Revised Inspiral Rates for Double Neutron Star Systems Chunglee Kim (Northwestern)

Revised Inspiral Rates for Double Neutron Star Systems Chunglee Kim (Northwestern). with Vicky Kalogera (Northwestern) & Duncan R. Lorimer (Manchester) 8 th Gravitational Wave Data Analysis Workshop Milwaukee, WI (Dec. 17, 2003). ? PSR J0737-3039 (Burgay et al. 2003)

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240 views • 14 slides

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J0737 - PowerPoint PPT Presentation

Lecture1. Structure of Neutron Stars

Neutron Star (Mostly Pulsar) Masses

Revised Inspiral Rates for Double Neutron Star Systems Chunglee Kim (Northwestern)