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GRB Afterglow Spectra

GRB Afterglow Spectra. Daniel Perley Astro 250 19 September* 2005. * International Talk Like a Pirate Day. Background GRB Standard Model Relativistic Shock Energy Deposition Proton Energy Electron Energy Electron Distribution Magnetic Energy

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Cosmic collisions or how most of the structure forms in the Universe

Cosmic collisions or how most of the structure forms in the Universe. Galaxy NCG 1365 Credit: AAO. Pleiades open cluster of stars Credit: Nasa. Hercules Cluster Credit: V. Andersen (U. of Alabama, KPNO). Gravity, the main force in the Universe. It is all a matter of attraction:

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References: Hunter, D.A., Hawley, W.N., & Gallagher, J.S. 1993, AJ 106, 179

1 arcmin. Figure 2: H a emission from NGC 1569 (Hunter et al. 1993). Note the numerous filaments extending far into the halo and the prominent H a arm in the west.

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Shocked gas - PowerPoint PPT Presentation

GRB Afterglow Spectra

Cosmic collisions or how most of the structure forms in the Universe

References: Hunter, D.A., Hawley, W.N., &amp; Gallagher, J.S. 1993, AJ 106, 179

References: Hunter, D.A., Hawley, W.N., & Gallagher, J.S. 1993, AJ 106, 179