Pulsars and their environments

Pulsars and their environments. May 11-13, 2015, Orléans. The workshop MODE-SNR-PWN will bring together three different communities interested in the physics of neutron stars the neutron star observers, the supernova remnants and pulsar wind nebulae observers and the theoreticians microphysics and macroscopic modelisation. It is supported by the PNHE, Orléans University and the COST activity NewCompStar. Which models shall be developed to analyze the new data? Observation at different wave lengths.

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NewCompStar Exploring fundamental physics with compact stars

Exploring fundamental physics with compact stars. Compact Stars in a nutshell. Was officially started on Nov. 25 2013 and represents the natural evolution of an ESF-funded RPN, CompStar. General information about COST Actions can be found on the network webpages. The rules and regulations for a COST Actions are summarized in the Vademecum. The Charter of NewCompstar is embodied in its Memorandum of Understanding. What is a compact star? .

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Pulsars and their environments

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Pulsars and their environments. May 11-13, 2015, Orléans. The workshop MODE-SNR-PWN will bring together three different communities interested in the physics of neutron stars the neutron star observers, the supernova remnants and pulsar wind nebulae observers and the theoreticians microphysics and macroscopic modelisation. It is supported by the PNHE, Orléans University and the COST activity NewCompStar. Which models shall be developed to analyze the new data? Observation at different wave lengths.

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The domain mode.obspm.fr states the following, "May 11-13, 2015, Orléans." I observed that the website also said " The workshop MODE-SNR-PWN will bring together three different communities interested in the physics of neutron stars the neutron star observers, the supernova remnants and pulsar wind nebulae observers and the theoreticians microphysics and macroscopic modelisation." They also stated " It is supported by the PNHE, Orléans University and the COST activity NewCompStar. Which models shall be developed to analyze the new data? Observation at different wave lengths."

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