21–25 Oct 2013
MPE
Europe/Berlin timezone

Session

Cosmic rays and their impact on the ISM

25 Oct 2013, 09:00
MPE

MPE

Gießenbachstraße 1 85748 Garching

Conveners

Cosmic rays and their impact on the ISM

  • Ellen Gould Zweibel

Presentation materials

There are no materials yet.

  1. Tsuyoshi Inoue (Aoyama Gakuin University)
    25/10/2013, 09:00
    review talk
  2. Sabrina Casanova (MPIK, Heidelberg)
    25/10/2013, 09:40
    contributed talk
    We 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...
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  3. Philipp Girichidis (MPA Garching)
    25/10/2013, 09:55
    contributed talk
    We 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...
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  4. Miwa Goto (USM/LMU)
    25/10/2013, 10:10
    contributed talk
    Cosmic 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...
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  5. Ruizhi Yang (Purple Mountain Observatory)
    25/10/2013, 10:25
    contributed talk
    We 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...
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