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Documents 1 Molecules in galaxies at all redshifts 1. How to observe the H 2 component? 2. Molecular component...

Slide 11 Molecules in galaxies at all redshifts 1. How to observe the H 2 component? 2. Molecular component of the Milky Way 3. Fractal Structure 4. Formation of the fractal,…

Documents Deuterated molecules: a chemical filter for recently evaporated gas Francesco Fontani (INAF-OAA) C.....

Slide 1Deuterated molecules: a chemical filter for recently evaporated gas Francesco Fontani (INAF-OAA) C. Codella, C. Ceccarelli, B. Lefloch, M.E. Palumbo … et al. Slide…

Documents Complete Ionisation of the Neutral Gas in the Hosts of High Redshift AGN As Traced Through HI and...

Slide 1 Steve Curran Complete Ionisation of the Neutral Gas in the Hosts of High Redshift AGN As Traced Through HI and MgII Absorption 0 Or why the SKA won’t detect HI…

Documents Molecules in galaxies at all redshifts 1. How to observe the H 2 component?

Molecules in galaxies at all redshifts 1. How to observe the H2 component? 2. Molecular component of the Milky Way 3. Fractal Structure 4. Formation of the fractal, shear,…

Documents A note on units: Column densities of air or water vapor are in: moles/m 2

Disussion of dispersion etc. (especially between wavelength bands) and fringe-tracking - Jeff Meisner A note on units: Column densities of air or water vapor are in: moles/m2…