Conveners
Cosmic rays and their impact on the ISM
- Ellen Gould Zweibel
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Tsuyoshi Inoue (Aoyama Gakuin University)25/10/2013, 09:00review talk
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Sabrina Casanova (MPIK, Heidelberg)25/10/2013, 09:40contributed talkWe solve the transport equations of cosmic rays inside a molecular cloud assuming an arbitrary energy and space dependent diffusion coefficient. Cosmic rays penetrating the cloud produce gamma-ray emission through pp collisions with the ambient gas. For small diffusion coefficients inside the cloud we expect the gamma-ray spectrum from the cloud to be harder than the Galactic diffuse emission...Go to contribution page
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Philipp Girichidis (MPA Garching)25/10/2013, 09:55contributed talkWe explore the impact of cosmic rays (CR) on the structure of the ISM, the turbulence in the Galactic disk, and how/to what extent cosmic rays drive Galactic outflows. We include the production of cosmic rays in SN remnants in a stratified box and follow the coupled system of gas and cosmic ray fluid self-consistently in three-dimensional adaptive mesh refinement simulations. The coupled...Go to contribution page
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Miwa Goto (USM/LMU)25/10/2013, 10:10contributed talkCosmic ray is a unique place that high-energy astrophysics meets low-energy chemistry. The ion molecule H3+ is the best chemical probe of the cosmic ray ionization rate, because of the simplicity of the chemical process. Meanwhile, a new gamma-ray observation identified a point like source near Sgr A*. To produce the gamma-ray flux discovered by HESS collaboration by a neutral pion decay, one...Go to contribution page
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Ruizhi Yang (Purple Mountain Observatory)25/10/2013, 10:25contributed talkWe report the results of our study on the energy spectra and absolute fluxes of cosmic rays (CRs) in the Local Galaxy based on three-year $\gamma$-ray observations of ten nearby giant molecular clouds (GMCs) belongs to the Gould Belt, with the Fermi Large Area Telescope (LAT). The $\gamma$-ray signals obtained with high statistical significance allow the determination of $\gamma$-ray spectra...Go to contribution page