The physics of the star formation process in M51

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20cm (VLA ABCD)

Infrared Emission, ISM and Star Formation!

Dumas Gaelle, February 24 th 2010!

Radio Maps!

VLA + single dish Effelsberg

Resolution ~ 2” (80pc)

3.6cm (VLA CD+Eff)

6cm (VLA BCD+Eff)

Künstlicher Stern über dem Calar Alto (Teil 2)

Near-infrared luminosity function of galaxies in distant clusters

Max-Planck-Institut für Astronomie - Jahresbericht 2007

Max-Planck-Institut für Astronomie - Jahresbericht 2009

Where lies the Peak of the Brown Dwarf Binary Separation ...

Sterrewacht Leiden - FTP Directory Listing

Annual Report 2011 Max Planck Institute for Astronomy

20cm (VLA ABCD) Infrared Emission, ISM and Star Formation! Dumas Gaelle, February 24 th 2010! Radio Maps! VLA + single dish Effelsberg Resolution ~ 2” (80pc) 3.6cm (VLA CD+Eff) 6cm (VLA BCD+Eff)

Infrared Emission, ISM and Star Formation! Dumas Gaelle, February 24 th 2010! • MiPS (Calzetti et al. 05) Resolution = 6” MIPS 24μm Spitzer Map! • MIPS + HiRes (Velusamy et al. 08) Resolution = 2.4” HIRES

Page 1 and 2: Infrared Emission, ISM and Star For
Page 3 and 4: Radio/IR relation! • Global (de J
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The physics of the star formation process in M51

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