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The Magellanic Clouds and dSph satellites. Vienna, April 10-12

Ram pressure induced star formation. Chiara Mastropietro LMU Munich A. Burkert (LMU) & B.Moore (UniZH). The Magellanic Clouds and dSph satellites. Vienna, April 10-12. LMC Parkes HI survey (Stavely-Smith et al. 2003). HI TIDAL FEATURES ??. 20 kpc. 20 kpc.

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181 views • 11 slides

Open questions & Working plan 1. C6D6 (Claudia, Cristian , Giusepe and Kevin)

Open questions & Working plan 1. C6D6 (Claudia, Cristian , Giusepe and Kevin) 1.1. Reported differences between normalization to gold at thermal and 4.9 eV (maybe related to beam interception factor AND/OR neutron flux of 2011 vs. 2010) obtain normalization from gold @ 200 keV

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104 views • 2 slides

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Mgas 0 - PowerPoint PPT Presentation

The Magellanic Clouds and dSph satellites. Vienna, April 10-12

Open questions &amp; Working plan 1. C6D6 (Claudia, Cristian , Giusepe and Kevin)

Open questions & Working plan 1. C6D6 (Claudia, Cristian , Giusepe and Kevin)